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Chang CS, Kuo CL, Huang CS, Cheng YS, Lin SS, Liu CS. The relationship between pulse pressure with plasma PCSK9 and interleukin-6 among patients with acute ischemic stroke and dyslipidemia. Brain Res 2022; 1795:148080. [PMID: 36088960 DOI: 10.1016/j.brainres.2022.148080] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/23/2022] [Revised: 09/02/2022] [Accepted: 09/05/2022] [Indexed: 11/29/2022]
Abstract
BACKGROUND AND PURPOSE A high plasma concentration of proprotein convertase subtilisin/kexin type 9 is characteristic of a prothrombotic state in cardiovascular diseases. Elevated inflammatory markers, such as interleukin-6, are associated with worse outcomes after ischemic stroke. We aimed to study the role of plasma PCSK9 and IL-6 in acute ischemic stroke with dyslipidemia. METHODS We divided 123 enrolled patients with first-ever acute ischemic stroke into normotensive and high blood pressure groups and further into high and low pulse pressure subgroups. Clinical characteristics and inflammatory and metabolic parameters, including plasma PCSK9 and IL-6, were recorded. RESULTS After the analysis of the normotensive and BP groups, there were positive correlations between PP and carotid stenosis (P = 0.031) and plaque numbers (P = 0.013) and between National Institute of Health Stroke Scale scores (P = 0.019) and carotid stenosis severity (P = 0.021) and resistance index (P = 0.04). There was a significant association between plasma cholesterol and PCSK9 (P = 0.044) in the low PP subgroup and IL-6 (P = 0.042) in the high PP subgroup. CONCLUSIONS Our findings indicated that plasma PCSK9 levels were associated with the low PP subgroup, while IL-6 was associated with the high PP subgroup. Dyslipidemia control is also necessary for those who had a stroke and who have high PP. Further investigation to assess the role of PCSK9 and IL-6 in patients with stroke is required for early treatment and secondary prevention.
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Affiliation(s)
- Chen-Shu Chang
- Department of Neurology, Changhua Christian Hospital, Changhua 500, Taiwan; Department of Medical Laboratory Science and Biotechnology, Central-Taiwan University of Science of Technology, Taichung 406, Taiwan; Department of Medical Imaging and Radiological Sciences, Central-Taiwan University of Science of Technology, Taichung 406, Taiwan
| | - Chen-Ling Kuo
- Vascular Medicine and Diabetes Research Center, Changhua Christian Hospital, Changhua 500, Taiwan
| | - Ching-Shan Huang
- Center of Regenerative Medicine and Tissue Repair, Changhua Christian Hospital, Changhua 500, Taiwan
| | - Yu-Shan Cheng
- Vascular Medicine and Diabetes Research Center, Changhua Christian Hospital, Changhua 500, Taiwan
| | - Song-Shei Lin
- Department of Medical Imaging and Radiological Sciences, Central-Taiwan University of Science of Technology, Taichung 406, Taiwan
| | - Chin-San Liu
- Department of Neurology, Changhua Christian Hospital, Changhua 500, Taiwan; Graduate Institute of Integrated Medicine, China Medical University, Taichung 404, Taiwan; Vascular and Genomic Center, Institute of ATP, Changhua Christian Hospital, Changhua 500, Taiwan; Department of Post-Baccalaureate Medicine, College of Medicine, National Chung Hsing University, Taichung 402, Taiwan.
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Ade PAR, Ahmed Z, Amiri M, Barkats D, Thakur RB, Bischoff CA, Beck D, Bock JJ, Boenish H, Bullock E, Buza V, Cheshire JR, Connors J, Cornelison J, Crumrine M, Cukierman A, Denison EV, Dierickx M, Duband L, Eiben M, Fatigoni S, Filippini JP, Fliescher S, Goeckner-Wald N, Goldfinger DC, Grayson J, Grimes P, Hall G, Halal G, Halpern M, Hand E, Harrison S, Henderson S, Hildebrandt SR, Hilton GC, Hubmayr J, Hui H, Irwin KD, Kang J, Karkare KS, Karpel E, Kefeli S, Kernasovskiy SA, Kovac JM, Kuo CL, Lau K, Leitch EM, Lennox A, Megerian KG, Minutolo L, Moncelsi L, Nakato Y, Namikawa T, Nguyen HT, O'Brient R, Ogburn RW, Palladino S, Prouve T, Pryke C, Racine B, Reintsema CD, Richter S, Schillaci A, Schwarz R, Schmitt BL, Sheehy CD, Soliman A, Germaine TS, Steinbach B, Sudiwala RV, Teply GP, Thompson KL, Tolan JE, Tucker C, Turner AD, Umiltà C, Vergès C, Vieregg AG, Wandui A, Weber AC, Wiebe DV, Willmert J, Wong CL, Wu WLK, Yang H, Yoon KW, Young E, Yu C, Zeng L, Zhang C, Zhang S. Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season. Phys Rev Lett 2021; 127:151301. [PMID: 34678017 DOI: 10.1103/physrevlett.127.151301] [Citation(s) in RCA: 18] [Impact Index Per Article: 6.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/21/2021] [Accepted: 08/12/2021] [Indexed: 06/13/2023]
Abstract
We present results from an analysis of all data taken by the BICEP2, Keck Array, and BICEP3 CMB polarization experiments up to and including the 2018 observing season. We add additional Keck Array observations at 220 GHz and BICEP3 observations at 95 GHz to the previous 95/150/220 GHz dataset. The Q/U maps now reach depths of 2.8, 2.8, and 8.8 μK_{CMB} arcmin at 95, 150, and 220 GHz, respectively, over an effective area of ≈600 square degrees at 95 GHz and ≈400 square degrees at 150 and 220 GHz. The 220 GHz maps now achieve a signal-to-noise ratio on polarized dust emission exceeding that of Planck at 353 GHz. We take auto- and cross-spectra between these maps and publicly available WMAP and Planck maps at frequencies from 23 to 353 GHz and evaluate the joint likelihood of the spectra versus a multicomponent model of lensed ΛCDM+r+dust+synchrotron+noise. The foreground model has seven parameters, and no longer requires a prior on the frequency spectral index of the dust emission taken from measurements on other regions of the sky. This model is an adequate description of the data at the current noise levels. The likelihood analysis yields the constraint r_{0.05}<0.036 at 95% confidence. Running maximum likelihood search on simulations we obtain unbiased results and find that σ(r)=0.009. These are the strongest constraints to date on primordial gravitational waves.
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Affiliation(s)
- P A R Ade
- School of Physics and Astronomy, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - Z Ahmed
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
| | - M Amiri
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
| | - D Barkats
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - R Basu Thakur
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - C A Bischoff
- Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221, USA
| | - D Beck
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - J J Bock
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - H Boenish
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - E Bullock
- Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Buza
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - J R Cheshire
- Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - J Connors
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - J Cornelison
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - M Crumrine
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - A Cukierman
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - E V Denison
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - M Dierickx
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - L Duband
- Service des Basses Températures, Commissariat à l'Energie Atomique, 38054 Grenoble, France
| | - M Eiben
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - S Fatigoni
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
| | - J P Filippini
- Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
- Department of Astronomy, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
| | - S Fliescher
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - N Goeckner-Wald
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - D C Goldfinger
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - J Grayson
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - P Grimes
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - G Hall
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - G Halal
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - M Halpern
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
| | - E Hand
- Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221, USA
| | - S Harrison
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - S Henderson
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
| | - S R Hildebrandt
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - G C Hilton
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - J Hubmayr
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - H Hui
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - K D Irwin
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - J Kang
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - K S Karkare
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - E Karpel
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - S Kefeli
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - S A Kernasovskiy
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - J M Kovac
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
- Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
| | - C L Kuo
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - K Lau
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - E M Leitch
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - A Lennox
- Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
| | - K G Megerian
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - L Minutolo
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - L Moncelsi
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - Y Nakato
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - T Namikawa
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan
| | - H T Nguyen
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - R O'Brient
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - R W Ogburn
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - S Palladino
- Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221, USA
| | - T Prouve
- Service des Basses Températures, Commissariat à l'Energie Atomique, 38054 Grenoble, France
| | - C Pryke
- Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - B Racine
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
- Aix-Marseille Université, CNRS/IN2P3, CPPM, Marseille 13288, France
| | - C D Reintsema
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - S Richter
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - A Schillaci
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - R Schwarz
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - B L Schmitt
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - C D Sheehy
- Physics Department, Brookhaven National Laboratory, Upton, New York 11973, USA
| | - A Soliman
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - T St Germaine
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
- Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
| | - B Steinbach
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - R V Sudiwala
- School of Physics and Astronomy, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - G P Teply
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - K L Thompson
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - J E Tolan
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - C Tucker
- School of Physics and Astronomy, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A D Turner
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - C Umiltà
- Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221, USA
- Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
| | - C Vergès
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - A G Vieregg
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
- Department of Physics, Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA
| | - A Wandui
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - A C Weber
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - D V Wiebe
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada
| | - J Willmert
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C L Wong
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
- Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
| | - W L K Wu
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
| | - H Yang
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - K W Yoon
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - E Young
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - C Yu
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - L Zeng
- Center for Astrophysics, Harvard & Smithsonian, Cambridge, Massachusetts 02138, USA
| | - C Zhang
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - S Zhang
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
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Abstract
Introduction During the COVID-19 pandemic, pre-existing dementia was associated with a 3x increase in risk of hospitalisation and (25.6%) of COVID-19 related deaths had dementia. However, it is unclear whether people living with dementia are at higher risk of COVID-19 due to dementia or whether there may be a biologically plausible link between dementia and COVID-19. The ApoE e4 allele is highly associated with dementia. We aimed to test the COVID-19 risk associated with dementia and the association between ApoE e4e4 allele and COVID-19 with the aim of clarifying biological vulnerability. Methods UK Biobank (England) participants baseline (2006 to 2010), plus secondary care data to 2017. Separate analysis tested dementia and ApoE genotype association with COVID-19 status (16th March-31st May 2020) or mortality (to March 31, 2020, plus incomplete deaths from April, 2020) in logistic models, adjusted for demographics and technical covariates. Results In 269,070 participants aged 65+, including 507(0.2%) hospitalized COVID-19 patients, those with pre-existing dementia were at increased risk of being hospitalized for COVID-19 (OR = 3.50 95% CI 1.93 to 6.34) and also for COVID-19 and death (OR = 7.30 95% CI 3.28–16.21). In 375,689 European-ancestry UKB participants, ApoE e4e4 homozygotes were more likely to be COVID-19 test positives (reaching genome-wide significance: OR = 2.24, 95% CI:1.72–2.93, p = 3.24 × 10–9) and of mortality with test-confirmed COVID-19 (OR = 4.29, 95% CI: 2.38–7.72, p = 1.22 × 10–6), compared to e3e3s homozygotes. The associations were little changed in subsets of participants who were free of diseases associated with ApoE e4 and COVID-19 severity. Conclusion Dementia was found to be disproportionally common in older adults who develop severe COVID-19. We have shown a plausible genetic pathway of increased COVID-19 risk with dementia, therefore suggesting that the positive association between dementia and COVID-19 is not just the result of high cases of COVID-19 in care homes.
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Affiliation(s)
- J Masoli
- University of Exeter Medical School; Royal Devon and Exeter NHS Trust; Center on Aging, University of Connecticut
| | - C L Kuo
- University of Exeter Medical School; Royal Devon and Exeter NHS Trust; Center on Aging, University of Connecticut
| | - J Atkins
- University of Exeter Medical School; Royal Devon and Exeter NHS Trust; Center on Aging, University of Connecticut
| | - L Pilling
- University of Exeter Medical School; Royal Devon and Exeter NHS Trust; Center on Aging, University of Connecticut
| | - J Delgado
- University of Exeter Medical School; Royal Devon and Exeter NHS Trust; Center on Aging, University of Connecticut
| | - G Kuchel
- University of Exeter Medical School; Royal Devon and Exeter NHS Trust; Center on Aging, University of Connecticut
| | - D Melzer
- University of Exeter Medical School; Royal Devon and Exeter NHS Trust; Center on Aging, University of Connecticut
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Chang CS, Kuo CL, Huang CS, Cheng YS, Lin SS, Liu CS. Association of cyclophilin A level and pulse pressure in predicting recurrence of cerebral infarction. Kaohsiung J Med Sci 2019; 36:122-128. [PMID: 31670477 DOI: 10.1002/kjm2.12143] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/27/2019] [Accepted: 09/22/2019] [Indexed: 12/26/2022] Open
Abstract
Cyclophilin A (CypA), secreted from vascular smooth muscle cells and inflammatory cells in response to oxidative stress, promotes vascular atherosclerosis and development of carotid stenosis. Increased concentration of plasma CypA in acute cerebral infarction was demonstrated clinically. The primary aim of this study was to investigate the prognostic impact between CypA level and outcome in patients with acute ischemic stroke. Admission serum CypA concentrations were detected in 66 acute cerebral infarction patients and in 52 healthy individuals. Inflammatory biomarkers, including high-sensitivity C-reactive protein, adhesion molecules, interleukins, and matrix-metalloproteases, were also assessed. We also examined the relationship between plasma biomarkers, blood pressure (BP), pulse pressure, the carotid artery velocity, the prognostic assessment with modified Rankin scale, and stroke recurrence. Plasma CypA concentration was higher on the first day of hospitalization in the high BP stroke group than in normal BP stroke group, which was statistically significant, which was observed even in the third month and sixth month follow-up outpatient periods. For stroke recurrence prediction, there was an important association between the higher (>60) pulse pressure on the seventh day of hospitalization and CypA level on the third month and sixth month follow-up outpatient periods. Our study revealed higher circulating serum levels of CypA in the hypertensive stroke group than in the non-hypertensive stroke group. We expect that elevated plasma CypA level and raised pulse pressure during hospitalization to become valuable biomarkers in predicting stroke recurrence in the sixth month assessment of acute cerebral infarction.
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Affiliation(s)
- Chen-Shu Chang
- Department of Neurology, Changhua Christian Hospital, Changhua, Taiwan.,Department of Medical Imaging and Radiological Sciences, Central-Taiwan University of Science and Technology, Taichung, Taiwan.,Department of Medical Laboratory Science and Biotechnology, Central-Taiwan University of Science and Technology, Taichung, Taiwan
| | - Chen-Ling Kuo
- Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua, Taiwan
| | - Ching-Shan Huang
- Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua, Taiwan
| | - Yu-Shan Cheng
- Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua, Taiwan
| | - Song-Shei Lin
- Department of Medical Imaging and Radiological Sciences, Central-Taiwan University of Science and Technology, Taichung, Taiwan
| | - Chin-San Liu
- Department of Neurology, Changhua Christian Hospital, Changhua, Taiwan.,Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua, Taiwan.,School of Chinese Medicine, Graduate Institute of Integrated Medicine, China Medical University, Taichung, Taiwan
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5
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Chang CS, Su SL, Kuo CL, Huang CS, Tseng WM, Lin SS, Liu CS. Cyclophilin A: A Predictive Biomarker of Carotid Stenosis in Cerebral Ischemic Stroke. Curr Neurovasc Res 2019; 15:111-119. [PMID: 29766804 DOI: 10.2174/1567202615666180516120959] [Citation(s) in RCA: 10] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/19/2018] [Revised: 04/10/2018] [Accepted: 04/12/2018] [Indexed: 11/22/2022]
Abstract
BACKGROUND Cyclophilin A plays a pathogenic role in the development and progression of atherosclerosis, which can be assessed by measuring carotid intima-media thickness. The primary aim of this study was to examine the interaction between plasma Cyclophilin A level and carotid intima-media thickness in patients with acute ischemic stroke. METHOD Plasma concentration of Cyclophilin A was measured on admission in 66 consecutive patients who had been hospitalized for acute cerebral stroke and in 52 case-control subjects without a history of acute stroke. Subjects in both groups also underwent ultrasound B-mode imaging to measure the mean and maximum intima-media thickness of the carotid artery. Inflammatory biomarkers including high-sensitivity C-reactive protein and fibrinogen were also assessed. RESULTS We found that the plasma concentration of Cyclophilin A was significantly higher in patients with acute ischemic stroke (p = 0.042). Increased Cyclophilin A was also correlated with carotid intima-media thickness in the patient group (p < 0.001). Among the risk factors for cerebral stroke examined in this study, only hypertension was significantly associated with plasma Cyclophilin A level. CONCLUSION Increased plasma Cyclophilin A levels might be involved in the pathophysiology of acute ischemic stroke and Cyclophilin A might serve as a biomarker in risk assessment of acute stroke patients.
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Affiliation(s)
- Chen-Shu Chang
- Department of Neurology, Changhua Christian Hospital, Changhua 500, Taiwan.,Department of Medical Laboratory Science and Biotechnology, Central-Taiwan University of Science and Technology, Taichung, Taiwan.,Department of Medical Imaging and Radiological Sciences, Central-Taiwan University of Science of Technology, Taichung 406, Taiwan
| | - Shih-Li Su
- Division of Endocrinology and Metabolism, Department of Internal Medicine, Diabetes Education Center, Changhua Christian Hospital, Changhua, Taiwan.,Institute of Medicine, Chung Shan Medical University, Taichung, Taiwan
| | - Chen-Ling Kuo
- Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua 500, Taiwan
| | - Ching-Shan Huang
- Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua 500, Taiwan
| | - Wan-Min Tseng
- Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua 500, Taiwan
| | - Song-Shei Lin
- Department of Medical Imaging and Radiological Sciences, Central-Taiwan University of Science of Technology, Taichung 406, Taiwan
| | - Chin-San Liu
- Department of Neurology, Changhua Christian Hospital, Changhua 500, Taiwan.,Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua 500, Taiwan.,School of Chinese Medicine, Graduate Institute of Integrated Medicine, China Medical University, Taichung 404, Taiwan
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Abstract
To find the associations of circulating cyclophilin A (CyP A) and CD147/EMMPRIN with renal outcomes in type 2 diabetes patients and possible pathogenesis involved. Total 131 patients were recruited since 2004. Glycated hemoglobin, blood glucose and urine albumin-creatinine ratio levels at baseline and every 3 months were measured. Plasma CyP A and CD147 were also measured at baseline. Patients were divided into two groups based upon the median level of the baseline plasma CyP A value: < 93.64 ng/mL (group A, n = 65), ≥ 93.64 ng/mL (group B, n = 66). The estimated glomerular filtration rate was calculated at each follow-up visit. Besides, mitochondrial function assay by cellular mitochondrial energy utility was studied when cells were exposed to glucose or exogenous CyP A or both. Multivariate analysis, using median level (93.64) ng/mL as the cut-off value, revealed that circulating CyP A and CD147 levels at baseline were associated with the baseline estimated glomerular filtration rate (eGFR) (p = .042 and p = .001 separately) in cross-sectional analysis. Longitudinally, higher baseline plasma CyP A level was also correlated to a rapid decline in eGFR (p = .016). The results were also significant when using the continuous plasma CyP A level (p = .003). In cells exposed to glucose, results of oxygen consumption rate (OCR) showed a significant reduction in basal respiration, maximal respiration and ATP production. Depressed OCR further occurred when incubated with both of CyP A and glucose. Plasma CyP A and CD147 can serve as indicators of renal disease progression in type 2 diabetes patients.
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Affiliation(s)
- Ping-Fang Chiu
- a School of Medicine , Chung Shan Medical University , Taichung , Taiwan.,b Nephrology Division, Department of Internal Medicine , Changhua Christian Hospital , Changhua , Taiwan.,c Vascular & Genomic Research Center , Changhua Christian Hospital , Changhua , Taiwan.,d Center of General Education , Tunghai University , Taiwan
| | - Shih-Li Su
- c Vascular & Genomic Research Center , Changhua Christian Hospital , Changhua , Taiwan.,d Center of General Education , Tunghai University , Taiwan
| | - Chun-Chieh Tsai
- b Nephrology Division, Department of Internal Medicine , Changhua Christian Hospital , Changhua , Taiwan
| | - Chia-Lin Wu
- b Nephrology Division, Department of Internal Medicine , Changhua Christian Hospital , Changhua , Taiwan
| | - Chen-Ling Kuo
- c Vascular & Genomic Research Center , Changhua Christian Hospital , Changhua , Taiwan
| | - Chew-Teng Kor
- e Division of Endocrinology and Metabolism, Department of Internal Medicine , Diabetes Education Center, Changhua Christian Hospital , Changhua , Taiwan
| | - Chia-Chu Chang
- a School of Medicine , Chung Shan Medical University , Taichung , Taiwan.,b Nephrology Division, Department of Internal Medicine , Changhua Christian Hospital , Changhua , Taiwan.,f Internal Medicine Research Center , Changhua Christian Hospital , Changhua , Taiwan
| | - Chin-San Liu
- a School of Medicine , Chung Shan Medical University , Taichung , Taiwan.,c Vascular & Genomic Research Center , Changhua Christian Hospital , Changhua , Taiwan.,g Department of Neurology , Changhua Christian Hospital , Changhua , Taiwan.,h Graduate Institute of Integrative Chinese and Western Medicine , China Medical University , Taichung , Taiwan
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7
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Ade PAR, Ahmed Z, Aikin RW, Alexander KD, Barkats D, Benton SJ, Bischoff CA, Bock JJ, Bowens-Rubin R, Brevik JA, Buder I, Bullock E, Buza V, Connors J, Cornelison J, Crill BP, Crumrine M, Dierickx M, Duband L, Dvorkin C, Filippini JP, Fliescher S, Grayson J, Hall G, Halpern M, Harrison S, Hildebrandt SR, Hilton GC, Hui H, Irwin KD, Kang J, Karkare KS, Karpel E, Kaufman JP, Keating BG, Kefeli S, Kernasovskiy SA, Kovac JM, Kuo CL, Larsen NA, Lau K, Leitch EM, Lueker M, Megerian KG, Moncelsi L, Namikawa T, Netterfield CB, Nguyen HT, O'Brient R, Ogburn RW, Palladino S, Pryke C, Racine B, Richter S, Schillaci A, Schwarz R, Sheehy CD, Soliman A, St Germaine T, Staniszewski ZK, Steinbach B, Sudiwala RV, Teply GP, Thompson KL, Tolan JE, Tucker C, Turner AD, Umiltà C, Vieregg AG, Wandui A, Weber AC, Wiebe DV, Willmert J, Wong CL, Wu WLK, Yang H, Yoon KW, Zhang C. Constraints on Primordial Gravitational Waves Using Planck, WMAP, and New BICEP2/Keck Observations through the 2015 Season. Phys Rev Lett 2018; 121:221301. [PMID: 30547645 DOI: 10.1103/physrevlett.121.221301] [Citation(s) in RCA: 28] [Impact Index Per Article: 4.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/02/2018] [Revised: 08/28/2018] [Indexed: 06/09/2023]
Abstract
We present results from an analysis of all data taken by the bicep2/Keck CMB polarization experiments up to and including the 2015 observing season. This includes the first Keck Array observations at 220 GHz and additional observations at 95 and 150 GHz. The Q and U maps reach depths of 5.2, 2.9, and 26 μK_{CMB} arcmin at 95, 150, and 220 GHz, respectively, over an effective area of ≈400 square degrees. The 220 GHz maps achieve a signal to noise on polarized dust emission approximately equal to that of Planck at 353 GHz. We take auto and cross spectra between these maps and publicly available WMAP and Planck maps at frequencies from 23 to 353 GHz. We evaluate the joint likelihood of the spectra versus a multicomponent model of lensed-ΛCDM+r+dust+synchrotron+noise. The foreground model has seven parameters, and we impose priors on some of these using external information from Planck and WMAP derived from larger regions of sky. The model is shown to be an adequate description of the data at the current noise levels. The likelihood analysis yields the constraint r_{0.05}<0.07 at 95% confidence, which tightens to r_{0.05}<0.06 in conjunction with Planck temperature measurements and other data. The lensing signal is detected at 8.8σ significance. Running a maximum likelihood search on simulations we obtain unbiased results and find that σ(r)=0.020. These are the strongest constraints to date on primordial gravitational waves.
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Affiliation(s)
- P A R Ade
- School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom
| | - Z Ahmed
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
| | - R W Aikin
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - K D Alexander
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - D Barkats
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - S J Benton
- Department of Physics, Princeton University, Princeton, New Jersey 08544, USA
| | - C A Bischoff
- Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221, USA
| | - J J Bock
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - R Bowens-Rubin
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - J A Brevik
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - I Buder
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - E Bullock
- Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Buza
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
- Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
| | - J Connors
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - J Cornelison
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - B P Crill
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - M Crumrine
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - M Dierickx
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - L Duband
- Service des Basses Températures, Commissariat à l'Energie Atomique, 38054 Grenoble, France
| | - C Dvorkin
- Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
| | - J P Filippini
- Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
- Department of Astronomy, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
| | - S Fliescher
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - J Grayson
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - G Hall
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - M Halpern
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, V6T 1Z1, Canada
| | - S Harrison
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - S R Hildebrandt
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - G C Hilton
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - H Hui
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - K D Irwin
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - J Kang
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - K S Karkare
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - E Karpel
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - J P Kaufman
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - B G Keating
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - S Kefeli
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - S A Kernasovskiy
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - J M Kovac
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
- Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
| | - C L Kuo
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - N A Larsen
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - K Lau
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - E M Leitch
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - M Lueker
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - K G Megerian
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - L Moncelsi
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - T Namikawa
- Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei 10617, Taiwan
| | - C B Netterfield
- Department of Physics, University of Toronto, Toronto, Ontario, M5S 1A7, Canada
- Canadian Institute for Advanced Research, Toronto, Ontario, M5G 1Z8, Canada
| | - H T Nguyen
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - R O'Brient
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - R W Ogburn
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - S Palladino
- Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221, USA
| | - C Pryke
- Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - B Racine
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - S Richter
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - A Schillaci
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - R Schwarz
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C D Sheehy
- Physics Department, Brookhaven National Laboratory, Upton, New York 11973, USA
| | - A Soliman
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - T St Germaine
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - Z K Staniszewski
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - B Steinbach
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - R V Sudiwala
- School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom
| | - G P Teply
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - K L Thompson
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - J E Tolan
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - C Tucker
- School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom
| | - A D Turner
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - C Umiltà
- Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221, USA
| | - A G Vieregg
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
- Department of Physics, Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA
| | - A Wandui
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - A C Weber
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - D V Wiebe
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, V6T 1Z1, Canada
| | - J Willmert
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C L Wong
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
- Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
| | - W L K Wu
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - H Yang
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - K W Yoon
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Rd, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - C Zhang
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
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8
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Dambska M, Labrador EB, Kuo CL, Weinstein DA. Prevention of complications in glycogen storage disease type Ia with optimization of metabolic control. Pediatr Diabetes 2017; 18:327-331. [PMID: 28568353 DOI: 10.1111/pedi.12540] [Citation(s) in RCA: 31] [Impact Index Per Article: 4.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 02/03/2017] [Revised: 03/23/2017] [Accepted: 04/20/2017] [Indexed: 11/29/2022] Open
Abstract
Prior to 1971, type Ia glycogen storage disease was marked by life-threatening hypoglycemia, lactic acidosis, severe failure to thrive, and developmental delay. With the introduction of continuous feeds in the 1970s and cornstarch in the 1980s, the prognosis improved, but complications almost universally developed. Changes in the management of type Ia glycogen storage disease have resulted in improved metabolic control, and this manuscript reviews the increasing evidence that complications can be delayed or prevented with optimal metabolic control as previously was seen in diabetes.
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Affiliation(s)
- M Dambska
- Glycogen Storage Disease Program, Connecticut Children's Medical Center, Hartford, Connecticut
| | - E B Labrador
- Glycogen Storage Disease Program, Connecticut Children's Medical Center, Hartford, Connecticut
| | - C L Kuo
- Department of Community Medicine and Health Care, University of Connecticut School of Medicine, Farmington, Connecticut.,Connecticut Institute for Clinical and Translational Science, Farmington, Connecticut
| | - D A Weinstein
- Glycogen Storage Disease Program, Connecticut Children's Medical Center, Hartford, Connecticut.,Department of Pediatrics, University of Connecticut School of Medicine, Farmington, Connecticut
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9
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Kuo CL, Tsai TL, Chang-Liao KS, Chao JH. Development of separation techniques for analysis of Nb-94 in radwaste samples. Appl Radiat Isot 2017; 128:165-170. [PMID: 28728069 DOI: 10.1016/j.apradiso.2017.07.016] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/01/2016] [Revised: 02/21/2017] [Accepted: 07/10/2017] [Indexed: 11/20/2022]
Abstract
A chemical separation technique for removing interfering gamma-ray radionuclides by combined precipitation of Nb pentoxide and anion exchange was proposed, thereby allowing detection of trace 94Nb in low-level radwastes. The detection limit for 94Nb was improved by a factor of 10-103, and the scaling factor (94Nb/60Co) of the radwastes was estimated to be less than 10-5. This technique can be used for low-level radwaste classification and power reactor decommissioning.
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Affiliation(s)
- C L Kuo
- Institute of Nuclear Engineering and Science, National Tsing Hua University, Hsinchu 30013, Taiwan ROC; Department of Nuclear Medicine, Hsinchu Mackay Memorial Hospital, Hsinchu 30071, Taiwan ROC
| | - T L Tsai
- Chemistry Division, Institute of Nuclear Energy Research, Longtan 32546, Taiwan ROC
| | - K S Chang-Liao
- Institute of Nuclear Engineering and Science, National Tsing Hua University, Hsinchu 30013, Taiwan ROC
| | - J H Chao
- Nuclear Science and Technology Development Center, National Tsing Hua University, Hsinchu 30013, Taiwan ROC.
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10
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Huang CH, Kuo CL, Huang CS, Liu CS, Chang CC. Depleted Leukocyte Mitochondrial DNA Copy Number Correlates With Unfavorable Left Ventricular Volumetric and Spherical Shape Remodeling in Acute Myocardial Infarction After Primary Angioplasty. Circ J 2017. [PMID: 28626147 DOI: 10.1253/circj.cj-17-0088] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Abstract
BACKGROUND Left ventricular (LV) shape influences LV systolic function. It is possible to assess LV shape using 3-D echocardiography sphericity index (SI). Maintaining mitochondrial DNA copy number (MCN) is important for preserving mitochondrial function and LV systolic function after acute myocardial infarction (AMI). Information is limited, however, regarding the relationship between leukocyte MCN and the subsequent change in LV shape after AMI.Methods and Results:Fifty-five AMI patients undergoing primary angioplasty were recruited. Plasma MCN was measured before primary angioplasty using quantitative polymerase chain reaction. 3-D echocardiography measurement of SI was performed at baseline, and at 1-, 3-, and 6-month follow-up. AMI subjects with MCN lower than the median had a higher 6-month SI and LV volume compared with those with higher MCN. Baseline echocardiographic parameters were similar between the 2 groups. MCN was negatively correlated with 3- and 6-month SI, and 3- and 6-month LV volume. On multiple linear regression analysis, baseline plasma MCN could predict LV SI and LV volume at 6 months after primary angioplasty for AMI, even after adjusting for traditional prognostic factors. CONCLUSIONS In AMI patients, higher plasma leukocyte MCN at baseline was associated with favorable LV shape and remodeling at 6-month follow-up. Plasma leukocyte MCN may provide a novel prognostic biomarker for LV remodeling after AMI.
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Affiliation(s)
- Ching-Hui Huang
- Division of Cardiology, Department of Internal Medicine, Changhua Christian Hospital.,Institute of Statistics and Information Science, National Changhua University of Education.,School of Medicine, College of Medicine, Kaohsiung Medical University.,Department of Beauty Science and Graduate Institute of Beauty Science Technology, Chienkuo Technology University
| | - Chen-Ling Kuo
- Vascular and Genomic Center, Changhua Christian Hospital
| | | | - Chin-San Liu
- Vascular and Genomic Center, Changhua Christian Hospital.,Department of Neurology, Changhua Christian Hospital
| | - Chia-Chu Chang
- Department of Nephrology, Changhua Christian Hospital.,Medical Research Center, Department of Internal Medicine, Changhua Christian Hospital.,School of Medicine, Chung Shan Medical University
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11
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Huang CH, Kuo CL, Huang CS, Tseng WM, Lian IB, Chang CC, Liu CS. High plasma coenzyme Q10 concentration is correlated with good left ventricular performance after primary angioplasty in patients with acute myocardial infarction. Medicine (Baltimore) 2016; 95:e4501. [PMID: 27495100 PMCID: PMC4979854 DOI: 10.1097/md.0000000000004501] [Citation(s) in RCA: 9] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 01/28/2016] [Revised: 06/20/2016] [Accepted: 07/13/2016] [Indexed: 01/11/2023] Open
Abstract
Exogenous administration of coenzyme Q10 (CoQ10) has been shown in experimental models to have a protective effect against ischemia-reperfusion injury. However, it is unclear whether follow-up plasma CoQ10 concentration is prognostic of left ventricular (LV) performance after primary balloon angioplasty in patients with acute ST segment elevation myocardial infarction (STEMI).We prospectively recruited 55 patients with STEMI who were treated with primary coronary balloon angioplasty. Plasma CoQ10 concentrations were measured before primary angioplasty (baseline) and 3 days, 7 days, and 1 month after STEMI using high-performance liquid chromatography. Echocardiography was performed at baseline and at 6-month follow-up. The control group comprised 54 healthy age- and sex-matched volunteers.Serial circulating CoQ10 concentrations significantly decreased with time in the STEMI group. The LV ejection fraction at 6-month follow-up positively correlated with the 1-month plasma CoQ10 tertile. Higher plasma CoQ10 concentrations at 1 month were associated with favorable LV remodeling and systolic function 6 months after STEMI. Multiple linear regression analysis showed that changes in CoQ10 concentrations at 1-month follow-up were predictive of LV systolic function 6 months after STEMI. Changes in CoQ10 concentrations correlated negatively with baseline oxidized low-density lipoprotein and fibrinogen concentrations and correlated positively with leukocyte mitochondrial copy number at baseline.Patients with STEMI who had higher plasma CoQ10 concentrations 1 month after primary angioplasty had better LV performance at 6-month follow-up. In addition, higher plasma CoQ10 concentration was associated with lower grade inflammatory and oxidative stress status. Therefore, plasma CoQ10 concentration may serve as a novel prognostic biomarker of LV systolic function after revascularization therapy for acute myocardial infarction.
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Affiliation(s)
- Ching-Hui Huang
- Division of Cardiology, Department of Internal Medicine, Changhua Christian Hospital
- Institute of Statistics and Information Science, National Changhua University of Education
| | | | | | | | - Ie Bin Lian
- Institute of Statistics and Information Science, National Changhua University of Education
| | - Chia-Chu Chang
- Division of Nephrology, Department of Internal Medicine, Changhua Christian Hospital, Changhua
- School of Medicine, Chung Shan Medical University, Taichung
| | - Chin-San Liu
- Vascular and Genomic Research Center
- Department of Neurology, Changhua Christian Hospital, Changhua
- Graduate Institute of Integrative Medicine, China Medical University, Taichung, Taiwan
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12
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Ade PAR, Ahmed Z, Aikin RW, Alexander KD, Barkats D, Benton SJ, Bischoff CA, Bock JJ, Bowens-Rubin R, Brevik JA, Buder I, Bullock E, Buza V, Connors J, Crill BP, Duband L, Dvorkin C, Filippini JP, Fliescher S, Grayson J, Halpern M, Harrison S, Hilton GC, Hui H, Irwin KD, Karkare KS, Karpel E, Kaufman JP, Keating BG, Kefeli S, Kernasovskiy SA, Kovac JM, Kuo CL, Leitch EM, Lueker M, Megerian KG, Netterfield CB, Nguyen HT, O'Brient R, Ogburn RW, Orlando A, Pryke C, Richter S, Schwarz R, Sheehy CD, Staniszewski ZK, Steinbach B, Sudiwala RV, Teply GP, Thompson KL, Tolan JE, Tucker C, Turner AD, Vieregg AG, Weber AC, Wiebe DV, Willmert J, Wong CL, Wu WLK, Yoon KW. Improved Constraints on Cosmology and Foregrounds from BICEP2 and Keck Array Cosmic Microwave Background Data with Inclusion of 95 GHz Band. Phys Rev Lett 2016; 116:031302. [PMID: 26849583 DOI: 10.1103/physrevlett.116.031302] [Citation(s) in RCA: 33] [Impact Index Per Article: 4.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/02/2015] [Indexed: 06/05/2023]
Abstract
We present results from an analysis of all data taken by the BICEP2 and Keck Array cosmic microwave background (CMB) polarization experiments up to and including the 2014 observing season. This includes the first Keck Array observations at 95 GHz. The maps reach a depth of 50 nK deg in Stokes Q and U in the 150 GHz band and 127 nK deg in the 95 GHz band. We take auto- and cross-spectra between these maps and publicly available maps from WMAP and Planck at frequencies from 23 to 353 GHz. An excess over lensed ΛCDM is detected at modest significance in the 95×150 BB spectrum, and is consistent with the dust contribution expected from our previous work. No significant evidence for synchrotron emission is found in spectra such as 23×95, or for correlation between the dust and synchrotron sky patterns in spectra such as 23×353. We take the likelihood of all the spectra for a multicomponent model including lensed ΛCDM, dust, synchrotron, and a possible contribution from inflationary gravitational waves (as parametrized by the tensor-to-scalar ratio r) using priors on the frequency spectral behaviors of dust and synchrotron emission from previous analyses of WMAP and Planck data in other regions of the sky. This analysis yields an upper limit r_{0.05}<0.09 at 95% confidence, which is robust to variations explored in analysis and priors. Combining these B-mode results with the (more model-dependent) constraints from Planck analysis of CMB temperature plus baryon acoustic oscillations and other data yields a combined limit r_{0.05}<0.07 at 95% confidence. These are the strongest constraints to date on inflationary gravitational waves.
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Affiliation(s)
- P A R Ade
- School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom
| | - Z Ahmed
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - R W Aikin
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - K D Alexander
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - D Barkats
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - S J Benton
- Department of Physics, University of Toronto, Toronto, Ontario, M5S 1A7, Canada
| | - C A Bischoff
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - J J Bock
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - R Bowens-Rubin
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - J A Brevik
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - I Buder
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - E Bullock
- Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Buza
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
- Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
| | - J Connors
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - B P Crill
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - L Duband
- Service des Basses Températures, Commissariat à l'Energie Atomique, 38054 Grenoble, France
| | - C Dvorkin
- Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
| | - J P Filippini
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Department of Physics, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA
| | - S Fliescher
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - J Grayson
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - M Halpern
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, V6T 1Z1, Canada
| | - S Harrison
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - G C Hilton
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - H Hui
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - K D Irwin
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - K S Karkare
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - E Karpel
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - J P Kaufman
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - B G Keating
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - S Kefeli
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - S A Kernasovskiy
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - J M Kovac
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
- Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
| | - C L Kuo
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - E M Leitch
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - M Lueker
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - K G Megerian
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - C B Netterfield
- Department of Physics, University of Toronto, Toronto, Ontario, M5S 1A7, Canada
- Canadian Institute for Advanced Research, Toronto, Ontario M5G 1Z8, Canada
| | - H T Nguyen
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - R O'Brient
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - R W Ogburn
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - A Orlando
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - C Pryke
- Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - S Richter
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - R Schwarz
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C D Sheehy
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - Z K Staniszewski
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - B Steinbach
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - R V Sudiwala
- School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom
| | - G P Teply
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - K L Thompson
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - J E Tolan
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - C Tucker
- School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom
| | - A D Turner
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - A G Vieregg
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
- Department of Physics, Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA
| | - A C Weber
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - D V Wiebe
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, V6T 1Z1, Canada
| | - J Willmert
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C L Wong
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
- Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
| | - W L K Wu
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - K W Yoon
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
- Department of Physics, Stanford University, Stanford, California 94305, USA
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Abstract
Cyclophilin A (CyPA), an oxidative stress-induced factor, was found to play an important role in the aneurysm formation. Our working hypothesis was that the plasma level of CyPA in ruptured intracranial aneurysm could predict the neurological outcome. From 2011 to 2013, a total of 36 patients with ruptured saccular intracranial aneurysm were recruited in our study. Before coil embolization, we draw blood samples at the orifice of a culprit aneurysm and in the remote peripheral vein for measurements of the CyPA levels. We utilized the modified Rankin scale 30 days after aneurysm rupture as the outcome measure. Generalized linear models were used to estimate the adjusted odds ratios of the poor neurological outcome given the presence of high plasma level of CyPA. The aneurysmal and venous CyPA levels were significantly associated with the initial clinical severity (P = 0.004 and 0.03, respectively) and 30-day outcome (P = 0.01 and 0.02, respectively). The aneurysmal CyPA levels modestly correlated with age and high Fisher grade (ρ = 0.39 and 0.41; P = 0.02 and 0.01, respectively). The aneurysmal CyPA levels strongly correlated with the venous counterpart (ρ = 0.89; P < 0.001). Patients with high levels of aneurysmal CyPA were 15.66 times (95% CI, 1.48-166.24; P = 0.02) more likely to have worse neurological outcome than those with the low levels after adjustment of the age, gender, and the documented confounding factors. High plasma level of CyPA is a significant prognostic biomarker for poor neurological outcome in patients with ruptured intracranial aneurysm.
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Affiliation(s)
- Hung-Wen Kao
- From the Department of Radiology, Tri-Service General Hospital, National Defense Medical Center, Taipei, Taiwan (HWK); Department of Biomedical Imaging and Radiological Sciences, National Yang-Ming University, Taipei, Taiwan (HWK, CPL); Department of Medical Imaging (KWL, WLC); Vascular and Genomic Center (KWL, WLC, CLK, CSH, WMT, CSL); Department of Neurology (CSL), Changhua Christian Hospital, Changhua, Taiwan; Graduate Institute of Integrative Medicine, China Medical University, Taichung, Taiwan (CSL); and Institute of Neuroscience, School of Life Science, National Yang-Ming University, Taipei, Taiwan (CPL)
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14
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Kao HW, Lee KW, Kuo CL, Huang CS, Tseng WM, Liu CS, Lin CP. Interleukin-6 as a Prognostic Biomarker in Ruptured Intracranial Aneurysms. PLoS One 2015; 10:e0132115. [PMID: 26176774 PMCID: PMC4503596 DOI: 10.1371/journal.pone.0132115] [Citation(s) in RCA: 27] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/01/2015] [Accepted: 06/10/2015] [Indexed: 11/17/2022] Open
Abstract
BACKGROUND Interleukin-6 (IL-6), a proinflammatory cytokine, was found to surge in the cerebral spinal fluid after aneurysmal subarachnoid hemorrhage (SAH). We hypothesized that the plasma level of IL-6 could be an independent biomarker in predicting clinical outcome of patients with ruptured intracranial aneurysm. METHODS We prospectively included 53 consecutive patients treated with platinum coil embolization of the ruptured intracranial aneurysm. Plasma IL-6 levels were measured in the blood samples at the orifices of the aneurysms and from peripheral veins. The outcome measure was the modified Rankin Scale one month after SAH. Multiple logistic regression analyses were used to evaluate the associations between the plasma IL-6 levels and the neurological outcome. RESULTS Significant risk factors for the poor outcome were old age, low Glasgow Coma Scale (GCS) on day 0, high Fisher grades, and high aneurysmal and venous IL-6 levels in univariate analyses. Aneurysmal IL-6 levels showed modest to moderate correlations with GCS on day 0, vasospasm grade and Fisher grade. A strong correlation was found between the aneurysmal and the corresponding venous IL-6 levels (ρ = 0.721; P<0.001). In the multiple logistic regression models, the poor 30-day mRS was significantly associated with high aneurysmal IL-6 level (OR, 17.97; 95% CI, 1.51-214.33; P = 0.022) and marginally associated with high venous IL-6 level (OR, 12.71; 95% CI, 0.90-180.35; P = 0.022) after adjusting for dichotomized age, GCS on day 0, and vasospasm and Fisher grades. CONCLUSIONS The plasma level of IL-6 is an independent prognostic biomarker that could be used to aid in the identification of patients at high-risk of poor neurological outcome after rupture of the intracranial aneurysm.
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Affiliation(s)
- Hung-Wen Kao
- Department of Radiology, Tri-Service General Hospital, National Defense Medical Center, Taipei, Taiwan; Department of Biomedical Imaging and Radiological Sciences, National Yang-Ming University, Taipei, Taiwan
| | - Kwo-Whei Lee
- Department of Medical Imaging, Changhua Christian Hospital, Changhua, Taiwan; Vascular and Genomic Center, Changhua Christian Hospital, Changhua, Taiwan
| | - Chen-Ling Kuo
- Vascular and Genomic Center, Changhua Christian Hospital, Changhua, Taiwan
| | - Ching-Shan Huang
- Vascular and Genomic Center, Changhua Christian Hospital, Changhua, Taiwan
| | - Wan-Min Tseng
- Vascular and Genomic Center, Changhua Christian Hospital, Changhua, Taiwan
| | - Chin-San Liu
- Vascular and Genomic Center, Changhua Christian Hospital, Changhua, Taiwan; Department of Neurology, Changhua Christian Hospital, Changhua, Taiwan; Graduate Institute of Integrative Medicine, China Medical University, Taichung, Taiwan
| | - Ching-Po Lin
- Department of Biomedical Imaging and Radiological Sciences, National Yang-Ming University, Taipei, Taiwan; Institute of Neuroscience, School of Life Science, National Yang-Ming University, Taipei, Taiwan
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15
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Ade PAR, Aghanim N, Ahmed Z, Aikin RW, Alexander KD, Arnaud M, Aumont J, Baccigalupi C, Banday AJ, Barkats D, Barreiro RB, Bartlett JG, Bartolo N, Battaner E, Benabed K, Benoît A, Benoit-Lévy A, Benton SJ, Bernard JP, Bersanelli M, Bielewicz P, Bischoff CA, Bock JJ, Bonaldi A, Bonavera L, Bond JR, Borrill J, Bouchet FR, Boulanger F, Brevik JA, Bucher M, Buder I, Bullock E, Burigana C, Butler RC, Buza V, Calabrese E, Cardoso JF, Catalano A, Challinor A, Chary RR, Chiang HC, Christensen PR, Colombo LPL, Combet C, Connors J, Couchot F, Coulais A, Crill BP, Curto A, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Delouis JM, Désert FX, Dickinson C, Diego JM, Dole H, Donzelli S, Doré O, Douspis M, Dowell CD, Duband L, Ducout A, Dunkley J, Dupac X, Dvorkin C, Efstathiou G, Elsner F, Enßlin TA, Eriksen HK, Falgarone E, Filippini JP, Finelli F, Fliescher S, Forni O, Frailis M, Fraisse AA, Franceschi E, Frejsel A, Galeotta S, Galli S, Ganga K, Ghosh T, Giard M, Gjerløw E, Golwala SR, González-Nuevo J, Górski KM, Gratton S, Gregorio A, Gruppuso A, Gudmundsson JE, Halpern M, Hansen FK, Hanson D, Harrison DL, Hasselfield M, Helou G, Henrot-Versillé S, Herranz D, Hildebrandt SR, Hilton GC, Hivon E, Hobson M, Holmes WA, Hovest W, Hristov VV, Huffenberger KM, Hui H, Hurier G, Irwin KD, Jaffe AH, Jaffe TR, Jewell J, Jones WC, Juvela M, Karakci A, Karkare KS, Kaufman JP, Keating BG, Kefeli S, Keihänen E, Kernasovskiy SA, Keskitalo R, Kisner TS, Kneissl R, Knoche J, Knox L, Kovac JM, Krachmalnicoff N, Kunz M, Kuo CL, Kurki-Suonio H, Lagache G, Lähteenmäki A, Lamarre JM, Lasenby A, Lattanzi M, Lawrence CR, Leitch EM, Leonardi R, Levrier F, Lewis A, Liguori M, Lilje PB, Linden-Vørnle M, López-Caniego M, Lubin PM, Lueker M, Macías-Pérez JF, Maffei B, Maino D, Mandolesi N, Mangilli A, Maris M, Martin PG, Martínez-González E, Masi S, Mason P, Matarrese S, Megerian KG, Meinhold PR, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Mitra S, Miville-Deschênes MA, Moneti A, Montier L, Morgante G, Mortlock D, Moss A, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Netterfield CB, Nguyen HT, Nørgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, O'Brient R, Ogburn RW, Orlando A, Pagano L, Pajot F, Paladini R, Paoletti D, Partridge B, Pasian F, Patanchon G, Pearson TJ, Perdereau O, Perotto L, Pettorino V, Piacentini F, Piat M, Pietrobon D, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Pratt GW, Prunet S, Pryke C, Puget JL, Rachen JP, Reach WT, Rebolo R, Reinecke M, Remazeilles M, Renault C, Renzi A, Richter S, Ristorcelli I, Rocha G, Rossetti M, Roudier G, Rowan-Robinson M, Rubiño-Martín JA, Rusholme B, Sandri M, Santos D, Savelainen M, Savini G, Schwarz R, Scott D, Seiffert MD, Sheehy CD, Spencer LD, Staniszewski ZK, Stolyarov V, Sudiwala R, Sunyaev R, Sutton D, Suur-Uski AS, Sygnet JF, Tauber JA, Teply GP, Terenzi L, Thompson KL, Toffolatti L, Tolan JE, Tomasi M, Tristram M, Tucci M, Turner AD, Valenziano L, Valiviita J, Van Tent B, Vibert L, Vielva P, Vieregg AG, Villa F, Wade LA, Wandelt BD, Watson R, Weber AC, Wehus IK, White M, White SDM, Willmert J, Wong CL, Yoon KW, Yvon D, Zacchei A, Zonca A. Joint analysis of BICEP2/keck array and Planck Data. Phys Rev Lett 2015; 114:101301. [PMID: 25815919 DOI: 10.1103/physrevlett.114.101301] [Citation(s) in RCA: 52] [Impact Index Per Article: 5.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/21/2015] [Indexed: 06/04/2023]
Abstract
We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2 and Keck Array have observed the same approximately 400 deg^{2} patch of sky centered on RA 0 h, Dec. -57.5°. The combined maps reach a depth of 57 nK deg in Stokes Q and U in a band centered at 150 GHz. Planck has observed the full sky in polarization at seven frequencies from 30 to 353 GHz, but much less deeply in any given region (1.2 μK deg in Q and U at 143 GHz). We detect 150×353 cross-correlation in B modes at high significance. We fit the single- and cross-frequency power spectra at frequencies ≥150 GHz to a lensed-ΛCDM model that includes dust and a possible contribution from inflationary gravitational waves (as parametrized by the tensor-to-scalar ratio r), using a prior on the frequency spectral behavior of polarized dust emission from previous Planck analysis of other regions of the sky. We find strong evidence for dust and no statistically significant evidence for tensor modes. We probe various model variations and extensions, including adding a synchrotron component in combination with lower frequency data, and find that these make little difference to the r constraint. Finally, we present an alternative analysis which is similar to a map-based cleaning of the dust contribution, and show that this gives similar constraints. The final result is expressed as a likelihood curve for r, and yields an upper limit r_{0.05}<0.12 at 95% confidence. Marginalizing over dust and r, lensing B modes are detected at 7.0σ significance.
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Affiliation(s)
- P A R Ade
- School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, United Kingdom
| | - N Aghanim
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
| | - Z Ahmed
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - R W Aikin
- California Institute of Technology, Pasadena, California, USA
| | - K D Alexander
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - M Arnaud
- Laboratoire AIM, IRFU/Service d'Astrophysique-CEA/DSM-CNRS-Université Paris Diderot, Bâtiment 709, CEA-Saclay, F-91191 Gif-sur-Yvette Cedex, France
| | - J Aumont
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
| | - C Baccigalupi
- SISSA, Astrophysics Sector, via Bonomea 265, 34136, Trieste, Italy
| | - A J Banday
- Université de Toulouse, UPS-OMP, IRAP, F-31028 Toulouse cedex 4, France
- CNRS, IRAP, 9 Avenue colonel Roche, BP 44346, F-31028 Toulouse cedex 4, France
| | - D Barkats
- Joint ALMA Observatory, Vitacura, Santiago, Chile
| | - R B Barreiro
- Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avenida de los Castros s/n, Santander, Spain
| | - J G Bartlett
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - N Bartolo
- Dipartimento di Fisica e Astronomia G. Galilei, Università degli Studi di Padova, via Marzolo 8, 35131 Padova, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, via Marzolo 8, I-35131 Padova, Italy
| | - E Battaner
- University of Granada, Departamento de Física Teórica y del Cosmos, Facultad de Ciencias, Granada, Spain
- University of Granada, Instituto Carlos I de Física Teórica y Computacional, Granada, Spain
| | - K Benabed
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
- UPMC Université de Paris 06, UMR7095, 98 bis Boulevard Arago, F-75014, Paris, France
| | - A Benoît
- Institut Néel, CNRS, Université Joseph Fourier Grenoble I, 25 rue des Martyrs, Grenoble, France
| | - A Benoit-Lévy
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
- UPMC Université de Paris 06, UMR7095, 98 bis Boulevard Arago, F-75014, Paris, France
- Department of Physics and Astronomy, University College London, London WC1E 6BT, United Kingdom
| | - S J Benton
- Department of Physics, University of Toronto, Toronto, Ontario, M5S 1A7, Canada
| | - J-P Bernard
- Université de Toulouse, UPS-OMP, IRAP, F-31028 Toulouse cedex 4, France
- CNRS, IRAP, 9 Avenue colonel Roche, BP 44346, F-31028 Toulouse cedex 4, France
| | - M Bersanelli
- Dipartimento di Fisica, Università degli Studi di Milano, Via Celoria, 16, Milano, Italy
- INAF/IASF Milano, Via E. Bassini 15, Milano, Italy
| | - P Bielewicz
- SISSA, Astrophysics Sector, via Bonomea 265, 34136, Trieste, Italy
- Université de Toulouse, UPS-OMP, IRAP, F-31028 Toulouse cedex 4, France
- CNRS, IRAP, 9 Avenue colonel Roche, BP 44346, F-31028 Toulouse cedex 4, France
| | - C A Bischoff
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - J J Bock
- California Institute of Technology, Pasadena, California, USA
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - A Bonaldi
- Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
| | - L Bonavera
- Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avenida de los Castros s/n, Santander, Spain
| | - J R Bond
- CITA, University of Toronto, 60 St. George Street, Toronto, Ontario M5S 3H8, Canada
| | - J Borrill
- Computational Cosmology Center, Lawrence Berkeley National Laboratory, Berkeley, California, USA
- Space Sciences Laboratory, University of California, Berkeley, California, USA
| | - F R Bouchet
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
- Sorbonne Université-UPMC, UMR7095, Institut d'Astrophysique de Paris, 98 bis Boulevard Arago, F-75014, Paris, France
| | - F Boulanger
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
| | - J A Brevik
- California Institute of Technology, Pasadena, California, USA
| | - M Bucher
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - I Buder
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - E Bullock
- Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C Burigana
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
- Dipartimento di Fisica e Scienze della Terra, Università di Ferrara, Via Saragat 1, 44122 Ferrara, Italy
- INFN, Sezione di Bologna, Via Irnerio 46, I-40126, Bologna, Italy
| | - R C Butler
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
| | - V Buza
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - E Calabrese
- Sub-Department of Astrophysics, University of Oxford, Keble Road, Oxford OX1 3RH, United Kingdom
| | - J-F Cardoso
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
- Laboratoire Traitement et Communication de l'Information, CNRS (UMR 5141) and Télécom ParisTech, 46 rue Barrault F-75634 Paris Cedex 13, France
| | - A Catalano
- Laboratoire de Physique Subatomique et Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, 53, rue des Martyrs, 38026 Grenoble Cedex, France
- LERMA, CNRS, Observatoire de Paris, 61 Avenue de l'Observatoire, Paris, France
| | - A Challinor
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
- Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom
- Centre for Theoretical Cosmology, DAMTP, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, United Kingdom
| | - R-R Chary
- Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, California 91125, USA
| | - H C Chiang
- Department of Physics, Princeton University, Princeton, New Jersey, USA
- Astrophysics & Cosmology Research Unit, School of Mathematics, Statistics & Computer Science, University of KwaZulu-Natal, Westville Campus, Private Bag X54001, Durban 4000, South Africa
| | - P R Christensen
- Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
- Discovery Center, Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
| | - L P L Colombo
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
- Department of Physics and Astronomy, Dana and David Dornsife College of Letter, Arts and Sciences, University of Southern California, Los Angeles, California 90089, USA
| | - C Combet
- Laboratoire de Physique Subatomique et Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, 53, rue des Martyrs, 38026 Grenoble Cedex, France
| | - J Connors
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - F Couchot
- LAL, Université Paris-Sud, CNRS/IN2P3, Orsay, France
| | - A Coulais
- LERMA, CNRS, Observatoire de Paris, 61 Avenue de l'Observatoire, Paris, France
| | - B P Crill
- California Institute of Technology, Pasadena, California, USA
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - A Curto
- Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avenida de los Castros s/n, Santander, Spain
- Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge CB3 0HE, United Kingdom
| | - F Cuttaia
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
| | - L Danese
- SISSA, Astrophysics Sector, via Bonomea 265, 34136, Trieste, Italy
| | - R D Davies
- Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
| | - R J Davis
- Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
| | - P de Bernardis
- Dipartimento di Fisica, Università La Sapienza, Piazzale Aldo Moro 2, Roma, Italy
| | - A de Rosa
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
| | - G de Zotti
- SISSA, Astrophysics Sector, via Bonomea 265, 34136, Trieste, Italy
- INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova, Italy
| | - J Delabrouille
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - J-M Delouis
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
- UPMC Université de Paris 06, UMR7095, 98 bis Boulevard Arago, F-75014, Paris, France
| | - F-X Désert
- IPAG: Institut de Planétologie et d'Astrophysique de Grenoble, Université Grenoble Alpes, IPAG, F-38000 Grenoble, France, CNRS, IPAG, F-38000 Grenoble, France
| | - C Dickinson
- Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
| | - J M Diego
- Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avenida de los Castros s/n, Santander, Spain
| | - H Dole
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
- Institut Universitaire de France, 103, bd Saint-Michel, 75005, Paris, France
| | - S Donzelli
- INAF/IASF Milano, Via E. Bassini 15, Milano, Italy
| | - O Doré
- California Institute of Technology, Pasadena, California, USA
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - M Douspis
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
| | - C D Dowell
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - L Duband
- Service des Basses Températures, Commissariat à l'Energie Atomique, 38054 Grenoble, France
| | - A Ducout
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
- Imperial College London, Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, United Kingdom
| | - J Dunkley
- Sub-Department of Astrophysics, University of Oxford, Keble Road, Oxford OX1 3RH, United Kingdom
| | - X Dupac
- European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la Cañada, Madrid, Spain
| | - C Dvorkin
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - G Efstathiou
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
| | - F Elsner
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
- UPMC Université de Paris 06, UMR7095, 98 bis Boulevard Arago, F-75014, Paris, France
- Department of Physics and Astronomy, University College London, London WC1E 6BT, United Kingdom
| | - T A Enßlin
- Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching, Germany
| | - H K Eriksen
- Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
| | - E Falgarone
- LERMA, CNRS, Observatoire de Paris, 61 Avenue de l'Observatoire, Paris, France
| | - J P Filippini
- California Institute of Technology, Pasadena, California, USA
- Department of Physics, University of Illinois at Urbana-Champaign, 1110 West Green Street, Urbana, Illinois, USA
| | - F Finelli
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
- INFN, Sezione di Bologna, Via Irnerio 46, I-40126, Bologna, Italy
| | - S Fliescher
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - O Forni
- Université de Toulouse, UPS-OMP, IRAP, F-31028 Toulouse cedex 4, France
- CNRS, IRAP, 9 Avenue colonel Roche, BP 44346, F-31028 Toulouse cedex 4, France
| | - M Frailis
- INAF-Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, Trieste, Italy
| | - A A Fraisse
- Department of Physics, Princeton University, Princeton, New Jersey, USA
| | - E Franceschi
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
| | - A Frejsel
- Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
| | - S Galeotta
- INAF-Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, Trieste, Italy
| | - S Galli
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
| | - K Ganga
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - T Ghosh
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
| | - M Giard
- Université de Toulouse, UPS-OMP, IRAP, F-31028 Toulouse cedex 4, France
- CNRS, IRAP, 9 Avenue colonel Roche, BP 44346, F-31028 Toulouse cedex 4, France
| | - E Gjerløw
- Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
| | - S R Golwala
- California Institute of Technology, Pasadena, California, USA
| | - J González-Nuevo
- SISSA, Astrophysics Sector, via Bonomea 265, 34136, Trieste, Italy
- Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avenida de los Castros s/n, Santander, Spain
| | - K M Górski
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
- Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland
| | - S Gratton
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
- Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom
| | - A Gregorio
- INAF-Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, Trieste, Italy
- Dipartimento di Fisica, Università degli Studi di Trieste, via Alfonso Valerio 2, Trieste, Italy
- INFN/National Institute for Nuclear Physics, Via Valerio 2, I-34127 Trieste, Italy
| | - A Gruppuso
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
| | - J E Gudmundsson
- Department of Physics, Princeton University, Princeton, New Jersey, USA
| | - M Halpern
- Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada
| | - F K Hansen
- Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
| | - D Hanson
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
- CITA, University of Toronto, 60 St. George Street, Toronto, Ontario M5S 3H8, Canada
- McGill Physics, Ernest Rutherford Physics Building, McGill University, 3600 rue University, Montréal, Quebec, H3A 2T8, Canada
| | - D L Harrison
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
- Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom
| | - M Hasselfield
- Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada
| | - G Helou
- California Institute of Technology, Pasadena, California, USA
| | | | - D Herranz
- Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avenida de los Castros s/n, Santander, Spain
| | - S R Hildebrandt
- California Institute of Technology, Pasadena, California, USA
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - G C Hilton
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - E Hivon
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
- UPMC Université de Paris 06, UMR7095, 98 bis Boulevard Arago, F-75014, Paris, France
| | - M Hobson
- Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge CB3 0HE, United Kingdom
| | - W A Holmes
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - W Hovest
- Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching, Germany
| | - V V Hristov
- California Institute of Technology, Pasadena, California, USA
| | - K M Huffenberger
- Department of Physics, Florida State University, Keen Physics Building, 77 Chieftan Way, Tallahassee, Florida, USA
| | - H Hui
- California Institute of Technology, Pasadena, California, USA
| | - G Hurier
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
| | - K D Irwin
- Department of Physics, Stanford University, Stanford, California 94305, USA
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
| | - A H Jaffe
- Imperial College London, Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, United Kingdom
| | - T R Jaffe
- Université de Toulouse, UPS-OMP, IRAP, F-31028 Toulouse cedex 4, France
- CNRS, IRAP, 9 Avenue colonel Roche, BP 44346, F-31028 Toulouse cedex 4, France
| | - J Jewell
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - W C Jones
- Department of Physics, Princeton University, Princeton, New Jersey, USA
| | - M Juvela
- Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, Helsinki, Finland
| | - A Karakci
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - K S Karkare
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - J P Kaufman
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - B G Keating
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - S Kefeli
- California Institute of Technology, Pasadena, California, USA
| | - E Keihänen
- Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, Helsinki, Finland
| | - S A Kernasovskiy
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - R Keskitalo
- Computational Cosmology Center, Lawrence Berkeley National Laboratory, Berkeley, California, USA
| | - T S Kisner
- Lawrence Berkeley National Laboratory, Berkeley, California, USA
| | - R Kneissl
- European Southern Observatory, ESO Vitacura, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile
- Atacama Large Millimeter/submillimeter Array, ALMA Santiago Central Offices, Alonso de Cordova 3107, Vitacura, Casilla 763 0355, Santiago, Chile
| | - J Knoche
- Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching, Germany
| | - L Knox
- Department of Physics, University of California, One Shields Avenue, Davis, California, USA
| | - J M Kovac
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - N Krachmalnicoff
- Dipartimento di Fisica, Università degli Studi di Milano, Via Celoria, 16, Milano, Italy
| | - M Kunz
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
- Département de Physique Théorique, Université de Genève, 24, Quai E. Ansermet, 1211 Genève 4, Switzerland
- African Institute for Mathematical Sciences, 6-8 Melrose Road, Muizenberg, Cape Town, South Africa
| | - C L Kuo
- Department of Physics, Stanford University, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
| | - H Kurki-Suonio
- Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, Helsinki, Finland
- Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland
| | - G Lagache
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
- Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326, 13388, Marseille, France
| | - A Lähteenmäki
- Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland
- Aalto University Metsähovi Radio Observatory and Department of Radio Science and Engineering, P.O. Box 13000, FI-00076 AALTO, Finland
| | - J-M Lamarre
- LERMA, CNRS, Observatoire de Paris, 61 Avenue de l'Observatoire, Paris, France
| | - A Lasenby
- Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom
- Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge CB3 0HE, United Kingdom
| | - M Lattanzi
- Dipartimento di Fisica e Scienze della Terra, Università di Ferrara, Via Saragat 1, 44122 Ferrara, Italy
| | - C R Lawrence
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - E M Leitch
- University of Chicago, Chicago, Illinois 60637, USA
| | - R Leonardi
- European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la Cañada, Madrid, Spain
| | - F Levrier
- LERMA, CNRS, Observatoire de Paris, 61 Avenue de l'Observatoire, Paris, France
| | - A Lewis
- Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, United Kingdom
| | - M Liguori
- Dipartimento di Fisica e Astronomia G. Galilei, Università degli Studi di Padova, via Marzolo 8, 35131 Padova, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, via Marzolo 8, I-35131 Padova, Italy
| | - P B Lilje
- Institute of Theoretical Astrophysics, University of Oslo, Blindern, Oslo, Norway
| | - M Linden-Vørnle
- DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 327, DK-2800 Kongens Lyngby, Denmark
| | - M López-Caniego
- Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avenida de los Castros s/n, Santander, Spain
- European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la Cañada, Madrid, Spain
| | - P M Lubin
- Department of Physics, University of California, Santa Barbara, California, USA
| | - M Lueker
- California Institute of Technology, Pasadena, California, USA
| | - J F Macías-Pérez
- Laboratoire de Physique Subatomique et Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, 53, rue des Martyrs, 38026 Grenoble Cedex, France
| | - B Maffei
- Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
| | - D Maino
- Dipartimento di Fisica, Università degli Studi di Milano, Via Celoria, 16, Milano, Italy
- INAF/IASF Milano, Via E. Bassini 15, Milano, Italy
| | - N Mandolesi
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
- Dipartimento di Fisica e Scienze della Terra, Università di Ferrara, Via Saragat 1, 44122 Ferrara, Italy
| | - A Mangilli
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
- LAL, Université Paris-Sud, CNRS/IN2P3, Orsay, France
| | - M Maris
- INAF-Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, Trieste, Italy
| | - P G Martin
- CITA, University of Toronto, 60 St. George Street, Toronto, Ontario M5S 3H8, Canada
| | - E Martínez-González
- Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avenida de los Castros s/n, Santander, Spain
| | - S Masi
- Dipartimento di Fisica, Università La Sapienza, Piazzale Aldo Moro 2, Roma, Italy
| | - P Mason
- California Institute of Technology, Pasadena, California, USA
| | - S Matarrese
- Dipartimento di Fisica e Astronomia G. Galilei, Università degli Studi di Padova, via Marzolo 8, 35131 Padova, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, via Marzolo 8, I-35131 Padova, Italy
- Gran Sasso Science Institute, INFN, viale F. Crispi 7, 67100L'Aquila, Italy
| | - K G Megerian
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - P R Meinhold
- Department of Physics, University of California, Santa Barbara, California, USA
| | - A Melchiorri
- Dipartimento di Fisica, Università La Sapienza, Piazzale Aldo Moro 2, Roma, Italy
- INFN, Sezione di Roma 1, Università di Roma Sapienza, Piazzale Aldo Moro 2, 00185, Roma, Italy
| | - L Mendes
- European Space Agency, ESAC, Planck Science Office, Camino bajo del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la Cañada, Madrid, Spain
| | - A Mennella
- Dipartimento di Fisica, Università degli Studi di Milano, Via Celoria, 16, Milano, Italy
- INAF/IASF Milano, Via E. Bassini 15, Milano, Italy
| | - M Migliaccio
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
- Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom
| | - S Mitra
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
- IUCAA, Post Bag 4, Ganeshkhind, Pune University Campus, Pune 411 007, India
| | - M-A Miville-Deschênes
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
- CITA, University of Toronto, 60 St. George Street, Toronto, Ontario M5S 3H8, Canada
| | - A Moneti
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
| | - L Montier
- Université de Toulouse, UPS-OMP, IRAP, F-31028 Toulouse cedex 4, France
- CNRS, IRAP, 9 Avenue colonel Roche, BP 44346, F-31028 Toulouse cedex 4, France
| | - G Morgante
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
| | - D Mortlock
- Imperial College London, Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, United Kingdom
| | - A Moss
- School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, United Kingdom
| | - D Munshi
- School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, United Kingdom
| | - J A Murphy
- National University of Ireland, Department of Experimental Physics, Maynooth, County Kildare, Ireland
| | - P Naselsky
- Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
- Discovery Center, Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
| | - F Nati
- Department of Physics, Princeton University, Princeton, New Jersey, USA
| | - P Natoli
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
- Dipartimento di Fisica e Scienze della Terra, Università di Ferrara, Via Saragat 1, 44122 Ferrara, Italy
- Agenzia Spaziale Italiana Science Data Center, Via del Politecnico snc, 00133, Roma, Italy
| | - C B Netterfield
- Department of Astronomy and Astrophysics, University of Toronto, 50 Saint George Street, Toronto, Ontario, Canada
| | - H T Nguyen
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - H U Nørgaard-Nielsen
- DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 327, DK-2800 Kongens Lyngby, Denmark
| | - F Noviello
- Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
| | - D Novikov
- Lebedev Physical Institute of the Russian Academy of Sciences, Astro Space Centre, 84/32 Profsoyuznaya st., Moscow, GSP-7, 117997, Russia
| | - I Novikov
- Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
- Lebedev Physical Institute of the Russian Academy of Sciences, Astro Space Centre, 84/32 Profsoyuznaya st., Moscow, GSP-7, 117997, Russia
| | - R O'Brient
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - R W Ogburn
- Department of Physics, Stanford University, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
| | - A Orlando
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - L Pagano
- Dipartimento di Fisica, Università La Sapienza, Piazzale Aldo Moro 2, Roma, Italy
- INFN, Sezione di Roma 1, Università di Roma Sapienza, Piazzale Aldo Moro 2, 00185, Roma, Italy
| | - F Pajot
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
| | - R Paladini
- Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, California 91125, USA
| | - D Paoletti
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
- INFN, Sezione di Bologna, Via Irnerio 46, I-40126, Bologna, Italy
| | - B Partridge
- Haverford College Astronomy Department, 370 Lancaster Avenue, Haverford, Pennsylvania, USA
| | - F Pasian
- INAF-Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, Trieste, Italy
| | - G Patanchon
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - T J Pearson
- California Institute of Technology, Pasadena, California, USA
- Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, California 91125, USA
| | - O Perdereau
- LAL, Université Paris-Sud, CNRS/IN2P3, Orsay, France
| | - L Perotto
- Laboratoire de Physique Subatomique et Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, 53, rue des Martyrs, 38026 Grenoble Cedex, France
| | - V Pettorino
- HGSFP and University of Heidelberg, Theoretical Physics Department, Philosophenweg 16, 69120, Heidelberg, Germany
| | - F Piacentini
- Dipartimento di Fisica, Università La Sapienza, Piazzale Aldo Moro 2, Roma, Italy
| | - M Piat
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
| | - D Pietrobon
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | | | - E Pointecouteau
- Université de Toulouse, UPS-OMP, IRAP, F-31028 Toulouse cedex 4, France
- CNRS, IRAP, 9 Avenue colonel Roche, BP 44346, F-31028 Toulouse cedex 4, France
| | - G Polenta
- Agenzia Spaziale Italiana Science Data Center, Via del Politecnico snc, 00133, Roma, Italy
- INAF-Osservatorio Astronomico di Roma, via di Frascati 33, Monte Porzio Catone, Italy
| | - N Ponthieu
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
- IPAG: Institut de Planétologie et d'Astrophysique de Grenoble, Université Grenoble Alpes, IPAG, F-38000 Grenoble, France, CNRS, IPAG, F-38000 Grenoble, France
| | - G W Pratt
- Laboratoire AIM, IRFU/Service d'Astrophysique-CEA/DSM-CNRS-Université Paris Diderot, Bâtiment 709, CEA-Saclay, F-91191 Gif-sur-Yvette Cedex, France
| | - S Prunet
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
- UPMC Université de Paris 06, UMR7095, 98 bis Boulevard Arago, F-75014, Paris, France
| | - C Pryke
- Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - J-L Puget
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
| | - J P Rachen
- Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching, Germany
- Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - W T Reach
- Universities Space Research Association, Stratospheric Observatory for Infrared Astronomy, MS 232-11, Moffett Field, California 94035, USA
| | - R Rebolo
- Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, La Laguna, Tenerife, Spain
- Consejo Superior de Investigaciones Científicas (CSIC), Madrid, Spain
- Departamento Astrofísica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
| | - M Reinecke
- Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching, Germany
| | - M Remazeilles
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
- Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
| | - C Renault
- Laboratoire de Physique Subatomique et Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, 53, rue des Martyrs, 38026 Grenoble Cedex, France
| | - A Renzi
- Dipartimento di Matematica, Università di Roma Tor Vergata, Via della Ricerca Scientifica, 1, Roma, Italy
- INFN, Sezione di Roma 2, Università di Roma Tor Vergata, Via della Ricerca Scientifica, 1, Roma, Italy
| | - S Richter
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - I Ristorcelli
- Université de Toulouse, UPS-OMP, IRAP, F-31028 Toulouse cedex 4, France
- CNRS, IRAP, 9 Avenue colonel Roche, BP 44346, F-31028 Toulouse cedex 4, France
| | - G Rocha
- California Institute of Technology, Pasadena, California, USA
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - M Rossetti
- Dipartimento di Fisica, Università degli Studi di Milano, Via Celoria, 16, Milano, Italy
- INAF/IASF Milano, Via E. Bassini 15, Milano, Italy
| | - G Roudier
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
- LERMA, CNRS, Observatoire de Paris, 61 Avenue de l'Observatoire, Paris, France
| | - M Rowan-Robinson
- Imperial College London, Astrophysics group, Blackett Laboratory, Prince Consort Road, London, SW7 2AZ, United Kingdom
| | - J A Rubiño-Martín
- Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, La Laguna, Tenerife, Spain
- Departamento Astrofísica, Universidad de La Laguna (ULL), E-38206 La Laguna, Tenerife, Spain
| | - B Rusholme
- Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, California 91125, USA
| | - M Sandri
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
| | - D Santos
- Laboratoire de Physique Subatomique et Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3, 53, rue des Martyrs, 38026 Grenoble Cedex, France
| | - M Savelainen
- Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, Helsinki, Finland
- Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland
| | - G Savini
- Optical Science Laboratory, University College London, Gower Street, London, United Kingdom
| | - R Schwarz
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - D Scott
- Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia, Canada
| | - M D Seiffert
- California Institute of Technology, Pasadena, California, USA
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - C D Sheehy
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
| | - L D Spencer
- School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, United Kingdom
| | - Z K Staniszewski
- California Institute of Technology, Pasadena, California, USA
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - V Stolyarov
- Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom
- Astrophysics Group, Cavendish Laboratory, University of Cambridge, J J Thomson Avenue, Cambridge CB3 0HE, United Kingdom
- Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnij Arkhyz, Zelenchukskiy region, Karachai-Cherkessian Republic, 369167, Russia
| | - R Sudiwala
- School of Physics and Astronomy, Cardiff University, Queens Buildings, The Parade, Cardiff, CF24 3AA, United Kingdom
| | - R Sunyaev
- Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching, Germany
- Space Research Institute (IKI), Russian Academy of Sciences, Profsoyuznaya Street, 84/32, Moscow, 117997, Russia
| | - D Sutton
- Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
- Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom
| | - A-S Suur-Uski
- Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, Helsinki, Finland
- Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland
| | - J-F Sygnet
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
| | - J A Tauber
- European Space Agency, ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
| | - G P Teply
- California Institute of Technology, Pasadena, California, USA
| | - L Terenzi
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
- Facoltà di Ingegneria, Università degli Studi e-Campus, Via Isimbardi 10, Novedrate (CO), 22060, Italy
| | - K L Thompson
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - L Toffolatti
- Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avenida de los Castros s/n, Santander, Spain
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
- Departamento de Física, Universidad de Oviedo, Avda. Calvo Sotelo s/n, Oviedo, Spain
| | - J E Tolan
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - M Tomasi
- Dipartimento di Fisica, Università degli Studi di Milano, Via Celoria, 16, Milano, Italy
- INAF/IASF Milano, Via E. Bassini 15, Milano, Italy
| | - M Tristram
- LAL, Université Paris-Sud, CNRS/IN2P3, Orsay, France
| | - M Tucci
- Département de Physique Théorique, Université de Genève, 24, Quai E. Ansermet, 1211 Genève 4, Switzerland
| | - A D Turner
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
- University of Chicago, Chicago, Illinois 60637, USA
| | - L Valenziano
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
| | - J Valiviita
- Department of Physics, Gustaf Hällströmin katu 2a, University of Helsinki, Helsinki, Finland
- Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland
| | - B Van Tent
- Laboratoire de Physique Théorique, Université Paris-Sud 11 & CNRS, Bâtiment 210, 91405 Orsay, France
| | - L Vibert
- Institut d'Astrophysique Spatiale, CNRS (UMR8617) Université Paris-Sud 11, Bâtiment 121, Orsay, France
| | - P Vielva
- Instituto de Física de Cantabria (CSIC-Universidad de Cantabria), Avenida de los Castros s/n, Santander, Spain
| | - A G Vieregg
- Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
- Department of Physics, Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA
| | - F Villa
- INAF/IASF Bologna, Via Gobetti 101, Bologna, Italy
| | - L A Wade
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - B D Wandelt
- Institut d'Astrophysique de Paris, CNRS (UMR7095), 98 bis Boulevard Arago, F-75014, Paris, France
- UPMC Université de Paris 06, UMR7095, 98 bis Boulevard Arago, F-75014, Paris, France
- Department of Physics, University of Illinois at Urbana-Champaign, 1110 West Green Street, Urbana, Illinois, USA
| | - R Watson
- Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
| | - A C Weber
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - I K Wehus
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA
| | - M White
- Department of Physics, University of California, Berkeley, California, USA
| | - S D M White
- Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching, Germany
| | - J Willmert
- School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C L Wong
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - K W Yoon
- Department of Physics, Stanford University, Stanford, California 94305, USA
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
| | - D Yvon
- DSM/Irfu/SPP, CEA-Saclay, F-91191 Gif-sur-Yvette Cedex, France
| | - A Zacchei
- INAF-Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, Trieste, Italy
| | - A Zonca
- Department of Physics, University of California, Santa Barbara, California, USA
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16
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Huang CH, Chang CC, Kuo CL, Huang CS, Lin CS, Liu CS. Decrease in plasma cyclophilin A concentration at 1 month after myocardial infarction predicts better left ventricular performance and synchronicity at 6 months: a pilot study in patients with ST elevation myocardial infarction. Int J Biol Sci 2015; 11:38-47. [PMID: 25552928 PMCID: PMC4278253 DOI: 10.7150/ijbs.10271] [Citation(s) in RCA: 17] [Impact Index Per Article: 1.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/05/2014] [Accepted: 11/05/2014] [Indexed: 01/12/2023] Open
Abstract
BACKGROUND Cyclophilin A (CyPA) concentration increases in acute coronary syndrome. In an animal model of acute myocardial infarction, administration of angiotensin-converting-enzyme inhibitor was associated with lower left ventricular (LV) CyPA concentration and improved LV performance. This study investigated the relationships between changes in plasma CyPA concentrations and LV remodeling in patients with ST-elevation myocardial infarction (STEMI). METHODS AND RESULTS We enrolled 55 patients who underwent percutaneous coronary intervention for acute STEMI. Plasma CyPA, matrix metalloproteinase (MMP), interleukin-6 and high-sensitivity C-reactive protein concentrations were measured at baseline and at one-month follow-up. Echocardiography was performed at baseline and at one-, three-, and six-month follow-up. Patients with a decrease in baseline CyPA concentration at one-month follow-up (n = 28) had a significant increase in LV ejection fraction (LVEF) (from 60.2 ± 11.5% to 64.6 ± 9.9%, p < 0. 001) and preserved LV synchrony at six months. Patients without a decrease in CyPA concentration at one month (n = 27) did not show improvement in LVEF and had a significantly increased systolic dyssynchrony index (SDI) (from 1.170 ± 0.510% to 1.637 ± 1.299%, p = 0.042) at six months. Multiple linear regression analysis showed a significant association between one-month CyPA concentration and six-month LVEF. The one-month MMP-2 concentration was positively correlated with one-month CyPA concentration and LV SDI. Conclusions : Decreased CyPA concentration at one-month follow-up after STEMI was associated with better LVEF and SDI at six months. Changes in CyPA, therefore, may be a prognosticator of patient outcome.
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Affiliation(s)
- Ching-Hui Huang
- 1. Division of Cardiology, Department of Internal Medicine, Changhua Christian Hospital, Changhua 500, Taiwan ; 2. Department of Biological Science and Technology, National Chiao Tung University, Hsinchu 300, Taiwan
| | - Chia-Chu Chang
- 3. Division of Nephrology, Department of Internal Medicine, Changhua Christian Hospital, Changhua 500, Taiwan ; 4. School of Medicine, Chung Shan Medical University, Taichung 404, Taiwan
| | - Chen-Ling Kuo
- 5. Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua 500, Taiwan
| | - Ching-Shan Huang
- 5. Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua 500, Taiwan
| | - Chih-Sheng Lin
- 2. Department of Biological Science and Technology, National Chiao Tung University, Hsinchu 300, Taiwan
| | - Chin-San Liu
- 5. Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua 500, Taiwan ; 6. Department of Neurology, Changhua Christian Hospital, Changhua 500, Taiwan ; 7. Graduate Institute of Integrative Medicine, China Medical University, Taichung 404, Taiwan
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17
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Lee KW, Tsai FY, Chen WL, Liu CK, Kuo CL. Intracranial venous hemodynamics and rupture of cerebral aneurysm. Neuroradiol J 2014; 27:703-9. [PMID: 25489894 DOI: 10.15274/nrj-2014-10091] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/07/2014] [Accepted: 08/24/2014] [Indexed: 11/12/2022] Open
Abstract
Many uncertain and inconsistent etiologies of cerebral aneurysmal rupture including a wide spectrum of factors have been reported. Our recent observation discloses the potential new factor of cerebral aneurysm rupture with cerebral venous pressure gradient. We retrospectively reviewed 52 cases treated with coil embolization with or without cerebral aneurysmal rupture. Seventeen males and 30 females were recruited in this study. Quantitative color-coded cerebral angiography was performed during coil therapeutic procedures to measure cerebral venous circulation. Ruptured cases had shorter and symmetrical cerebral venous circulation time (P <0.05). In addition, an asymmetrical venous outflow pattern was critical for aneurysmal rupture. Non-ruptured cases tended to have slower and asymmetrical cerebral venous circulation compared with rupture cases. Symmetrical and shorter cerebral venous circulation in the dysplasia venous outlet may be a potential new factor for cerebral aneurysm rupture.
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Affiliation(s)
- Kwo-Whei Lee
- Department of Medical Imaging, Vascular and Genomic Research Center, Changhua Christian Hospital; Taipei, Taiwan - Imaging Research Center, Taipei Medical University; Taipei, Taiwan - -
| | - Fong-Y Tsai
- Department of Medical Imaging, Changhua Christian Hospital; Taipei, Taiwan - Imaging Research Center, Taipei Medical University; Taipei, Taiwan
| | - Wei-Liang Chen
- Department of Medical Imaging, Vascular and Genomic Research Center, Changhua Christian Hospital; Taipei, Taiwan
| | - Chi-Kuang Liu
- Department of Medical Imaging, Vascular and Genomic Research Center, Changhua Christian Hospital; Taipei, Taiwan
| | - Chen-Ling Kuo
- Vascular and Genomic Research Center, Changhua Christian Hospital; Taipei, Taiwan
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18
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Ade PAR, Aikin RW, Barkats D, Benton SJ, Bischoff CA, Bock JJ, Brevik JA, Buder I, Bullock E, Dowell CD, Duband L, Filippini JP, Fliescher S, Golwala SR, Halpern M, Hasselfield M, Hildebrandt SR, Hilton GC, Hristov VV, Irwin KD, Karkare KS, Kaufman JP, Keating BG, Kernasovskiy SA, Kovac JM, Kuo CL, Leitch EM, Lueker M, Mason P, Netterfield CB, Nguyen HT, O'Brient R, Ogburn RW, Orlando A, Pryke C, Reintsema CD, Richter S, Schwarz R, Sheehy CD, Staniszewski ZK, Sudiwala RV, Teply GP, Tolan JE, Turner AD, Vieregg AG, Wong CL, Yoon KW. Detection of B-mode polarization at degree angular scales by BICEP2. Phys Rev Lett 2014; 112:241101. [PMID: 24996078 DOI: 10.1103/physrevlett.112.241101] [Citation(s) in RCA: 98] [Impact Index Per Article: 9.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/04/2014] [Indexed: 06/03/2023]
Abstract
We report results from the BICEP2 experiment, a cosmic microwave background (CMB) polarimeter specifically designed to search for the signal of inflationary gravitational waves in the B-mode power spectrum around ℓ∼80. The telescope comprised a 26 cm aperture all-cold refracting optical system equipped with a focal plane of 512 antenna coupled transition edge sensor 150 GHz bolometers each with temperature sensitivity of ≈300 μK(CMB)√s. BICEP2 observed from the South Pole for three seasons from 2010 to 2012. A low-foreground region of sky with an effective area of 380 square deg was observed to a depth of 87 nK deg in Stokes Q and U. In this paper we describe the observations, data reduction, maps, simulations, and results. We find an excess of B-mode power over the base lensed-ΛCDM expectation in the range 30 < ℓ < 150, inconsistent with the null hypothesis at a significance of >5σ. Through jackknife tests and simulations based on detailed calibration measurements we show that systematic contamination is much smaller than the observed excess. Cross correlating against WMAP 23 GHz maps we find that Galactic synchrotron makes a negligible contribution to the observed signal. We also examine a number of available models of polarized dust emission and find that at their default parameter values they predict power ∼(5-10)× smaller than the observed excess signal (with no significant cross-correlation with our maps). However, these models are not sufficiently constrained by external public data to exclude the possibility of dust emission bright enough to explain the entire excess signal. Cross correlating BICEP2 against 100 GHz maps from the BICEP1 experiment, the excess signal is confirmed with 3σ significance and its spectral index is found to be consistent with that of the CMB, disfavoring dust at 1.7σ. The observed B-mode power spectrum is well fit by a lensed-ΛCDM+tensor theoretical model with tensor-to-scalar ratio r = 0.20_(-0.05)(+0.07), with r = 0 disfavored at 7.0σ. Accounting for the contribution of foreground, dust will shift this value downward by an amount which will be better constrained with upcoming data sets.
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Affiliation(s)
- P A R Ade
- School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom
| | - R W Aikin
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - D Barkats
- Joint ALMA Observatory, Vitacura, Santiago, Chile
| | - S J Benton
- Department of Physics, University of Toronto, Toronto, Ontario, M5S 1A7, Canada
| | - C A Bischoff
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - J J Bock
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA and Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - J A Brevik
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - I Buder
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - E Bullock
- Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C D Dowell
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - L Duband
- Service des Basses Températures, Commissariat à l'Energie Atomique, 38054 Grenoble, France
| | - J P Filippini
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - S Fliescher
- Department of Physics, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - S R Golwala
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - M Halpern
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, V6T 1Z1, Canada
| | - M Hasselfield
- Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, V6T 1Z1, Canada
| | - S R Hildebrandt
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA and Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - G C Hilton
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - V V Hristov
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - K D Irwin
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA and Department of Physics, Stanford University, Stanford, California 94305, USA and Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
| | - K S Karkare
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - J P Kaufman
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - B G Keating
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - S A Kernasovskiy
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - J M Kovac
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - C L Kuo
- Department of Physics, Stanford University, Stanford, California 94305, USA and Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
| | - E M Leitch
- University of Chicago, Chicago, Illinois 60637, USA
| | - M Lueker
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - P Mason
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - C B Netterfield
- Department of Physics, University of Toronto, Toronto, Ontario, M5S 1A7, Canada and Canadian Institute for Advanced Research, Toronto, Ontario, M5G 1Z8, Canada
| | - H T Nguyen
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - R O'Brient
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - R W Ogburn
- Department of Physics, Stanford University, Stanford, California 94305, USA and Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
| | - A Orlando
- Department of Physics, University of California at San Diego, La Jolla, California 92093, USA
| | - C Pryke
- Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, Minnesota 55455, USA and Department of Physics, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C D Reintsema
- National Institute of Standards and Technology, Boulder, Colorado 80305, USA
| | - S Richter
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - R Schwarz
- Department of Physics, University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - C D Sheehy
- Department of Physics, University of Minnesota, Minneapolis, Minnesota 55455, USA and University of Chicago, Chicago, Illinois 60637, USA
| | - Z K Staniszewski
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA and Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - R V Sudiwala
- School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom
| | - G P Teply
- Department of Physics, California Institute of Technology, Pasadena, California 91125, USA
| | - J E Tolan
- Department of Physics, Stanford University, Stanford, California 94305, USA
| | - A D Turner
- Jet Propulsion Laboratory, Pasadena, California 91109, USA
| | - A G Vieregg
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA and University of Chicago, Chicago, Illinois 60637, USA
| | - C L Wong
- Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS 42, Cambridge, Massachusetts 02138, USA
| | - K W Yoon
- Department of Physics, Stanford University, Stanford, California 94305, USA and Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, California 94025, USA
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19
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Lee YL, Liu CE, Cho WL, Kuo CL, Cheng WL, Huang CS, Liu CS. Presence of cytomegalovirus DNA in leucocytes is associated with increased oxidative stress and subclinical atherosclerosis in healthy adults. Biomarkers 2014; 19:109-13. [PMID: 24446591 DOI: 10.3109/1354750x.2013.877967] [Citation(s) in RCA: 24] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/23/2022]
Abstract
OBJECTIVE Investigate the latent cytomegalovirus (CMV) infection as a biomarker of oxidative stress and atherosclerosis. METHODS Latent CMV infection was diagnosed in healthy individuals with PCR-evidence of CMV DNA in peripheral leucocytes. Oxidative stress and atherosclerosis were measured by mitochondrial DNA oxidative damage index (mtDNA(ΔCT)) and intima media thickness (IMT). RESULTS The CMV DNA positive subjects had a higher mean mtDNA(ΔCT) and greater IMT than subjects in the control group. CONCLUSIONS Presence of CMV DNA in leucocytes, as a marker of latent CMV infection, was associated with increased levels of oxidative stress and subclinical atherosclerosis in healthy adults.
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Affiliation(s)
- Yu-Lin Lee
- Department of Internal Medicine, Division of Infectious Diseases, Changhua Christian Hospital , Changhua , Taiwan
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20
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Chang CS, Su SL, Chang CC, Lee KW, Kuo CL, Huang CS, Tseng WM, Liu CS. Cyclophilin-A: a novel biomarker for untreated male essential hypertension. Biomarkers 2013; 18:716-20. [PMID: 24164594 DOI: 10.3109/1354750x.2013.847122] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/08/2023]
Abstract
Vascular cytokines, total nitrite, and cyclophilin-A (CyP-A) may be related to the pathogenesis of untreated hypertension. Forty males with normotensive and untreated essential hypertension were recruited in this cytokines survey. Body mass index (BMI), hyperlipidemia, and plasma CyP-A were increased in the hypertensive group (p < 0.05). However, only BMI (p = 0.022) and plasma CyP-A (p = 0.020) were found to be significant contributors to hypertension by multiple regression analysis. CyP-A was also positively correlated with systolic blood pressure (p = 0.029) and diastolic blood pressure (p = 0.047). These findings indicated that plasma CyP-A is a critical molecular biomarker in the early pathogenesis of essential hypertension.
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Affiliation(s)
- Chen-Shu Chang
- Department of Neurology, Changhua Christian Hospital , Changhua , Taiwan
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21
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Yu SC, Kuo CL, Huang CS, Chang CS, Wu SL, Su SL, Liu CS. Endogenous granulocyte colony-stimulating factor: a biomarker in acute ischemic stroke. Biomarkers 2012; 17:319-24. [PMID: 22440005 DOI: 10.3109/1354750x.2012.668712] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/13/2022]
Abstract
Granulocyte colony-stimulating factor (G-CSF) may protect ischemic brain injury either in animal or human. No studies have reported that endogenous G-CSF (enG-CSF) level is related to the severity of ischemic stroke. This study was designed to assess the severity of ischemic patients correlated with the alteration of enG-CSF on the 1st day after an ischemic event. Patient's plasma enG-CSF and scoring of National Institute of Health Stroke Scale were measured on the 1st day after ischemic stroke. The acute ischemic stroke could significantly induce enG-GCF secretion as compared with healthy control group (16.77 vs. 22.86 μg/L, p = 0.001). Elevated enG-CSF concentration was positively correlated with the severity of stroke patients on day 1 after the event (p = 0.006; Spearman correlation coefficient = 0.268). The enG-CSF is a good biomarker for prediction of severity of acute ischemic stroke.
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Affiliation(s)
- Shih-Chieh Yu
- Department of Neurology, Kuang-Tien General Hospital, Taichung, Taiwan
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22
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Huang CH, Su SL, Hsieh MC, Cheng WL, Chang CC, Wu HL, Kuo CL, Lin TT, Liu CS. Depleted Leukocyte Mitochondrial DNA Copy Number in Metabolic Syndrome. J Atheroscler Thromb 2011; 18:867-73. [DOI: 10.5551/jat.8698] [Citation(s) in RCA: 45] [Impact Index Per Article: 3.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022] Open
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23
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Liu CS, Soong BW, Lee YC, Chen WL, Kuo CL, Cheng WL, Huang CS, Lin WT. Gluten sensitivity: associated sporadic cerebellar ataxia in Taiwan. Acta Neurol Taiwan 2010; 19:263-269. [PMID: 21210327] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Subscribe] [Scholar Register] [Accepted: 06/08/2010] [Indexed: 05/30/2023]
Abstract
PURPOSE Gluten sensitivity (GS) is related to the pathogenesis of sporadic or hereditary ataxia. METHODS Total of 194 healthy controls and patients with either hereditary ataxia (n=207) or sporadic ataxia (n=361) were tested for the circulating gluten-related autoantibodies which serve as biomarkers to interpret the existence of GS. RESULTS The incidences of GS in each population were 1% in normal subjects, 2% in hereditary ataxia patients and 9% in sporadic ataxia patients. High serum level of anti-gliadin IgG/IgA and t-transglutaminase IgA were disclosed at the sporadic ataxia patients compared with normal subjects. However, the anti-gliadin IgG is more specific to the disease of sporadic ataxia. CONCLUSION Relatively higher incidence of GS was found in the population of sporadic ataxia patients but not in either normal subjects or hereditary ataxia patients in Taiwan. Anti-gliadin IgG still is a very powerful indicator to implicate the immune-related sporadic ataxia and we conclude that GS-related sporadic ataxia exists in Taiwan with linkage to autoimmune events.
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Affiliation(s)
- Chin-San Liu
- Department of Neurology, Vascular and Genomics Center, Changhua Christian Hospital, No. 135, Nanhsiao Street, Changhua 500, Taiwan.
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Liu CS, Lii CK, Chang LL, Kuo CL, Cheng WL, Su SL, Tsai CW, Chen HW. Atorvastatin increases blood ratios of vitamin E/low-density lipoprotein cholesterol and coenzyme Q10/low-density lipoprotein cholesterol in hypercholesterolemic patients. Nutr Res 2010; 30:118-24. [DOI: 10.1016/j.nutres.2010.01.007] [Citation(s) in RCA: 14] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/28/2009] [Revised: 01/07/2010] [Accepted: 01/21/2010] [Indexed: 10/19/2022]
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Yu YC, Kuo CL, Cheng WL, Liu CS, Hsieh M. Decreased antioxidant enzyme activity and increased mitochondrial DNA damage in cellular models of Machado-Joseph disease. J Neurosci Res 2009; 87:1884-91. [DOI: 10.1002/jnr.22011] [Citation(s) in RCA: 77] [Impact Index Per Article: 5.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/08/2022]
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Sun MJ, Cheng WL, Wei YH, Kuo CL, Sun S, Tsai HD, Lin HM, Liu CS. Low copy number and high 4977 deletion of mitochondrial DNA in uterosacral ligaments are associated with pelvic organ prolapse progression. Int Urogynecol J 2009; 20:867-72. [DOI: 10.1007/s00192-009-0871-4] [Citation(s) in RCA: 11] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/16/2008] [Accepted: 03/15/2009] [Indexed: 10/21/2022]
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Juo SHH, Liao YC, Kuo CL, Wang Y, Huang CS, Chiang HC, Liu CS. The MTHFR 677 C/T polymorphism influences plasma levels of adhesion molecules and nitric oxide. Thromb Res 2007; 121:549-54. [PMID: 17707074 DOI: 10.1016/j.thromres.2007.06.006] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/17/2007] [Revised: 05/23/2007] [Accepted: 06/14/2007] [Indexed: 10/22/2022]
Abstract
BACKGROUND Hyperhomocysteinemia is an independent risk factor for cardiovascular events. The T allele of 677 C/T polymorphism at the methylenetetrahydrofolate reductase (MTHFR) gene has been reported to induce mild hyperhomocysteinemia. In the present study, we investigated the relationship between this polymorphism and adhesion molecules and total nitric oxide (NOx). METHODS The adhesion molecules tested in the present study were soluble E-selectin (sE-selectin), vascular adhesion molecule (sVCAM), and intercellular adhesion molecule (sICAM). A total of 297 subjects had data on these atherosclerotic biomarkers and the MTHFR genotypes. The genetic effect was estimated in the multivariate regression models with adjustment of covariates. Homocysteine, folate, vitamin B6 and vitamin B12 levels were measured in 181 subjects for the test of association between the biomarkers and homocysteine levels. RESULTS The genotype distribution was in Hardy-Weinberg equilibrium. The sVCAM levels increased with the number of the T allele, while the NOx levels decreased with the number of the T allele. We found that the T allele was significantly associated with high sVCAM levels (p=0.002) and low NOx levels (p=0.011) in the regression models. The MTHFR genotypes were associated with homocysteine levels (p=0.031). Mild hyperhomocysteinemia (>12 micromol/L) was significantly associated with sVCAM levels (p=0.036). The NOx levels were lower in the hyperhomocysteinemia group than in the normal homocysteine group, but the difference was not significant. The genotypes were not significantly associated with either sE-selectin or sICAM. CONCLUSIONS The detrimental T allele exerted an additive effect to increase sVCAM and decrease NOx concentrations, which may contribute to atherosclerosis.
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Affiliation(s)
- Suh-Hang Hank Juo
- Graduate Institute of Medical Genetics, Kaohsiung Medical University, Department of Medical Research, Kaohsiung Medical University Hospital, Kaohsiung, Taiwan
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Liu CS, Chen CH, Chiang HC, Kuo CL, Huang CS, Cheng WL, Wei YH, Chen HW. B-group vitamins, MTHFR C677T polymorphism and carotid intima-media thickness in clinically healthy subjects. Eur J Clin Nutr 2007; 61:996-1003. [PMID: 17228344 DOI: 10.1038/sj.ejcn.1602606] [Citation(s) in RCA: 13] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Abstract
OBJECTIVE Plasma B-group vitamins and age may affect the carotid intima-media thickness (IMT) in subjects with different 677TT genotype of the methylenetetrahydrofolate reductase (MTHFR) gene. DESIGN A hospital-based cross-study. SETTING Genomic and Vascular Center, Changhua Christian Hospital, Changhua, Taiwan. SUBJECTS Five hundred and forty-one clinically healthy subjects. INTERVENTION Fasting plasma, homocysteine (Hcy), vitamin B(6), vitamin B(12), folate and B-mode carotid ultrasound. RESULTS MTHFR genotype, plasma concentrations of folate, vitamin B(6) and vitamin B(12) and age were significantly correlated to the plasma Hcy concentration. MTHFR 677TT carriers had higher concentrations of Hcy than did subjects with the CC and CT genotypes. Age, sex, body mass index and plasma Hcy were independent contributors to increase carotid IMT. However, with stratification by mean value of age and B-group vitamins concentrations, we found that at advanced age, lower plasma folate and vitamin B(12) were three risk factors involved in the enhancing effect of the MTHFR 677TT genotype on the increase of plasma Hcy and carotid IMT. CONCLUSION MTHFR 677TT-related carotid atherosclerosis was only identified in healthy elderly subjects with lower level of plasma folate and vitamin B(12). SPONSORSHIP Changhua Christian Hospital.
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Affiliation(s)
- C S Liu
- Department of Neurology, Chung Shan Medical University Hospital, Taichung, Taiwan.
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Liu CS, Chiang TH, Kuo CL, Ou CC, Lii CK, Sun-Hsun I, Wei YH, Chen HW. Contribution of plasma folic acid and homocysteine levels to the mean carotid intima media thickness in smokers. Nutr Res 2005. [DOI: 10.1016/j.nutres.2005.09.014] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/25/2022]
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Abstract
BACKGROUND From the deductive point of view, neurotransmitter receptors can be divided into categories such as cholinergic (muscarinic, nicotinic), adrenergic (alpha- and beta-), dopaminergic, serotoninergic (5-HT1 approximately 5-HT5), and histaminergic (H1 and H2). Selective agonists and antagonists of each receptor subtype can have specific useful therapeutic applications. For understanding the molecular mechanisms of action, an inductive method of analysis is useful. OBJECTIVE The aim of the present study is to examine the structure-activity relationships of agents acting on G-protein coupled receptors. METHOD Representative sets of G-PCR agonists and antagonists were identified from the literature and Medline [P.M. Walsh (2003) Physicians' Desk Reference; M.J. O'Neil (2001) The Merck Index]. The molecular weight (MW), calculated logarithm of octanol/water partition coefficient (C log P) and molar refraction (CMR), dipole moment (DM), E(lumo) (the energy of the lowest unoccupied molecular orbital, a measure of the electron affinity of a molecule and its reactivity as an electrophile), E(homo) (the energy of the highest occupied molecular orbital, related to the ionization potential of a molecule, and its reactivity as a nucleophile), and the total number of hydrogen bonds (H(b)) (donors and receptors), were chosen as molecular descriptors for SAR analyses. RESULTS The data suggest that not only do neurotransmitters share common structural features but their receptors belong to the same ensemble of G-protein coupled receptor with seven to eight transmembrane domains with their resultant dipoles in an antiparallel configuration. Moreover, the analysis indicates that the receptor exists in a dynamic equilibrium between the closed state and the open state. The energy needed to open the closed state is provided by the hydrolysis of GTP. A composite 3-D parameter frame setting of all the neurotransmitter agonists and antagonists are presented using MW, Hb and mu as independent variables. CONCLUSION It appears that all neurotransmitters examined in this study operate by a similar mechanism with the G-protein coupled receptors.
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MESH Headings
- Adrenergic Agonists/chemistry
- Adrenergic Agonists/classification
- Adrenergic Antagonists/chemistry
- Adrenergic Antagonists/classification
- Chemical Phenomena
- Chemistry, Physical
- Cholinergic Agonists/chemistry
- Cholinergic Agonists/classification
- Cholinergic Antagonists/chemistry
- Cholinergic Antagonists/classification
- Dopamine Agonists/chemistry
- Dopamine Agonists/classification
- Dopamine Agonists/pharmacology
- Dopamine Antagonists/chemistry
- Dopamine Antagonists/classification
- Dopamine Antagonists/pharmacology
- Histamine Agonists/chemistry
- Histamine Agonists/classification
- Histamine Agonists/pharmacology
- Histamine Antagonists/chemistry
- Histamine Antagonists/classification
- Histamine Antagonists/pharmacology
- Models, Biological
- Molecular Structure
- Neurotransmitter Agents/agonists
- Neurotransmitter Agents/antagonists & inhibitors
- Neurotransmitter Agents/chemistry
- Receptors, Adrenergic/classification
- Receptors, Adrenergic/drug effects
- Receptors, Adrenergic/physiology
- Receptors, Cholinergic/classification
- Receptors, Cholinergic/drug effects
- Receptors, Cholinergic/physiology
- Receptors, G-Protein-Coupled/drug effects
- Receptors, G-Protein-Coupled/physiology
- Receptors, Histamine/classification
- Receptors, Histamine/drug effects
- Receptors, Histamine/physiology
- Serotonin Antagonists/chemistry
- Serotonin Antagonists/classification
- Serotonin Antagonists/pharmacology
- Serotonin Receptor Agonists/chemistry
- Serotonin Receptor Agonists/classification
- Serotonin Receptor Agonists/pharmacology
- Structure-Activity Relationship
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Affiliation(s)
- C L Kuo
- School of Pharmacy, University of Southern California, 1985 Zonal Avenue, Los Angeles, CA 90089-9121, USA
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Liu CS, Chiang TH, Kuo CL, Lii CK, Ou CC, Wei YH, Chen HW. α-tocopherol is important to inhibit low-density lipoprotein oxidation in smokers. Nutr Res 2004. [DOI: 10.1016/j.nutres.2003.11.009] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/26/2022]
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Liu CS, Tsai CS, Kuo CL, Chen HW, Lii CK, Ma YS, Wei YH. Oxidative stress-related alteration of the copy number of mitochondrial DNA in human leukocytes. Free Radic Res 2004; 37:1307-17. [PMID: 14753755 DOI: 10.1080/10715760310001621342] [Citation(s) in RCA: 221] [Impact Index Per Article: 11.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/26/2022]
Abstract
The role of oxidative stress in the regulation of the copy number of mitochondrial DNA (mtDNA) in human leukocytes is unclear. In this study, we investigated the redox factors in plasma that may contribute to the alteration of mtDNA copy number in human leukocytes. A total of 156 healthy subjects of 25-80 years of age who exhibited no significant difference in the distribution of subpopulations of leukocytes in blood were recruited. Small-molecular-weight antioxidants and thiobarbituric acid reactive substances (TBARS) in plasma and 8-hydroxy-2'-deoxyguanosine (8-OHdG) and 4,977bp deletion of mtDNA in leukocytes were determined. The mtDNA copy number in leukocytes was determined by real-time PCR. The results showed that the copy number of mtDNA in leukocytes was changed with age in a biphasic manner that fits in a positively quadratic regression model (P = 0.001). Retinol (P = 0.005), non-protein thiols (P = 0.001) and ferritin (P = 0.004) in plasma and total glutathione in erythrocytes (P = 0.046) were the significant redox factors that correlated with the mtDNA copy number in leukocytes in a positive manner. By contrast, alpha-tocopherol levels in plasma (P = 0.001) and erythrocytes (P = 0.033) were negatively correlated with the mtDNA copy number in leukocytes. Three oxidative indices including the incidence of 4,977 bp deletion of mtDNA (P = 0.016) and 8-OHdG content in leukocytes (P = 0.003) and TBARS in plasma (P = 0.001) were all positively correlated with the copy number of mtDNA in leukocytes. Taken these findings together, we suggest that the copy number of mtDNA in leukocytes is affected by oxidative stress in blood circulation elicited by the alteration of plasma antioxidants/prooxidants and oxidative damage to DNA.
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Affiliation(s)
- Chin-San Liu
- Department of Neurology and Vascular and Genomic Research Center, Changhua Christian Hospital, Changhua 500, Taiwan
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Hysert PE, Mirand AL, Giovino GA, Cummings KM, Kuo CL. "At Face Value": age progression software provides personalised demonstration of the effects of smoking on appearance. Tob Control 2003; 12:238. [PMID: 12773741 PMCID: PMC1747721 DOI: 10.1136/tc.12.2.238] [Citation(s) in RCA: 15] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/04/2022]
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Abstract
OBJECTIVE A large number of structurally and functionally diverse compounds act as substrates or modulators of p-glycoprotein (p-gp). Some of them possess multiple drug resistance (MDR)-reversing activity, but only a small number of them have entered clinical study. In order to uncover the factors which exert a significant impact on the interaction between substrates/modulators and p-gp, we have performed structure-activity relationship (SAR) analyses, including molecular modelling, two-dimensional (2D) and three-dimensional (3D) parameter-frame-setting analysis, quantitative structure activity relationship (QSAR) analysis among substrates/modulators, as well as clinically promising MDR-reversing agents. METHODS The physicochemical parameters C log P, CMR and all regression equations were derived by using C log P version 4.0 and the latest CQSAR software, respectively. Molecular modelling and all other parameter calculations were performed by using HyperChem version 5.0 program, after geometry optimization and energy minimization using the AM1 semiempirical method. RESULTS SAR analyses indicate that MDR reversal activity is correlated with the lipophilicity (C log P), molecular weight (log Mw), longest chain (Nlc) of the molecule and the energy of the highest occupied orbital (Ehomo). In addition, the presence of a basic tertiary nitrogen atom in the structure is also an important contributor to p-gp inhibitory activity. Some separation in space is achieved for different subsets of p-gp substrates and inhibitors using Nlc, C log P and Ehomo as three independent parameters in the 3D-parameter-frame setting. CONCLUSION A highly effective p-gp modulator candidate should possess a log P value of 2.92 or higher, 18-atom-long or longer molecular axis, and a high Ehomo value, as well as at least one tertiary basic nitrogen atom. The results obtained may be useful in explaining drug-p-gp interactions for different compounds, including drug interactions and the development of new MDR chemosensitizers.
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Affiliation(s)
- R B Wang
- School of Pharmacy, Shandong University, Jinan, People's Republic of China
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35
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Chang CC, Manousakas I, Pu YR, Liang SM, Chen CH, Chen TS, Yu FM, Yang WH, Tong YC, Kuo CL. In vitro study of ultrasound based real-time tracking for renal stones in shock wave lithotripsy: Part II--a simulated animal experiment. J Urol 2002; 167:2594-7. [PMID: 11992093] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/24/2023]
Abstract
PURPOSE We have previously developed and reported an ultrasound based real-time tracking system for renal stones. In the current study we continued to verify the reliability of this tracking system by a simulated animal test. MATERIALS AND METHODS We used 13 prerecorded ultrasound stone trajectories to test the system. The real-time tracking system was implemented on the Litemed 9200 electrohydraulic lithotriptor (LiteMed Co., Taipei, Taiwan). An artificial stone and tap water were sealed in a balloon. The balloon was inserted into the pelvis of a pig kidney. While the kidney was affixed to and moved by a simulator, it was immersed in a specifically designed simulated animal model tank containing tap water. The stone was localized by ultrasound. The kidney was moved by the simulator according to a prerecorded stone trajectory. A total of 3,000 shock waves were delivered to the stone. For each recorded stone trajectory experiments were done under nontracking and tracking conditions. We performed tests of the fragment-to-weight ratio, which denotes the performance of a shock wave lithotriptor when fragmenting a stone. RESULTS The mean fragment-to-weight ratio was 55.3% +/- 25.9% in the nontracking and 100% +/- 0% in the tracking group. The difference in these 2 groups was statistically significant (paired t test p <0.01). CONCLUSIONS The ultrasound based real-time tracking system proved to improve the performance of a shock wave lithotriptor significantly when fragmenting stones in a simulated animal test. We believe that the tracking system would greatly reduce the number of shocks and time needed for treating renal stones.
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Affiliation(s)
- C C Chang
- Department of Urology, Institute of Biomedical Engineering, National Cheng Kung University and Hospital, Tainan, Taiwan, Republic of China
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Liu CS, Chen HW, Lii CK, Tsai CS, Kuo CL, Wei YH. Alterations of plasma antioxidants and mitochondrial DNA mutation in hair follicles of smokers. Environ Mol Mutagen 2002; 40:168-174. [PMID: 12355550 DOI: 10.1002/em.10105] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
Abstract
The effects of long-term smoking on mitochondrial DNA (mtDNA) deletions in hair follicles were investigated in subjects with different antioxidant capacity. Twenty-two male smokers with a smoking index of greater than 5 pack-years and without any known systemic diseases were recruited for this study. Forty healthy nonsmoking males were included as controls. We found that the concentrations of ascorbate and alpha-tocopherol and the activities of glutathione S-transferase (GST) and glutathione peroxidase in blood plasma were significantly decreased in smokers. The levels of glutathione and protein thiols in whole blood and the incidence of a 4,977 bp deletion of mtDNA (dmtDNA) in hair follicles were significantly increased in smokers. A significantly higher incidence of the 4,977 bp dmtDNA was found in smokers with plasma GST activity less than 5.66 U/l (OR = 7.2, P = 0.020). Using multiple covariate ANOVA and logistic regression, we found that age and low plasma GST activity were the only two risk factors for the 4,977 bp dmtDNA. These results suggest that smoking depletes antioxidants and causes mtDNA deletions and that plasma GST may play an important role in the preservation of the mitochondrial genome in tissue cells of smokers.
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Affiliation(s)
- Chin-San Liu
- Department of Neuroscience and Neurology, Changhua Christian Hospital, Changhua, Taiwan
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37
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Affiliation(s)
- C H Chen
- Changhua Show-Chwan Memorial Hospital, Changhua, Taiwan
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Sagare AP, Kuo CL, Chueh FS, Tsay HS. De novo regeneration of Scrophularia yoshimurae Yamazaki (Scrophulariaceae) and quantitative analysis of harpagoside, an iridoid glucoside, formed in aerial and underground parts of in vitro propagated and wild plants by HPLC. Biol Pharm Bull 2001; 24:1311-5. [PMID: 11725970 DOI: 10.1248/bpb.24.1311] [Citation(s) in RCA: 29] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/22/2022]
Abstract
A protocol for de novo regeneration and rapid micropropagation of Scrophularia yoshimurae (Scrophulariaceae) has been developed. Multiple shoot development was achieved by culturing the shoot-tip, leaf-base, stem-node and stem-internode explants on Murashige and Skoog (MS) medium supplemented with 4.44 microM N6-benzyladenine (BA) and 1.07 microM alpha-naphthaleneacetic acid (NAA). Stem-node and shoot-tip explants showed the highest response (100%) followed by stem-internode (74.4%) and leaf-base (7.7%) explants. The shoots were multiplied by subculturing on the same medium used for shoot induction. Shoots were rooted on growth regulator-free MS basal medium and the plantlets were transplanted to soil and acclimatized in the growth chamber. The content of harpagoside, a quantitatively predominant iridoid glycoside, in different plant material was determined by high performance liquid chromatography (HPLC). The analysis revealed that the content of harpagoside in the aerial and underground parts of S. yoshimurae was significantly higher than the marketed crude drug (underground parts of Scrophularia ningpoensis).
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Affiliation(s)
- A P Sagare
- Department of Agronomy Taiwan Agricultural Research Institute, Wufeng, Taichung
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Chang CC, Liang SM, Pu YR, Chen CH, Manousakas I, Chen TS, Kuo CL, Yu FM, Chu ZF. In vitro study of ultrasound based real-time tracking of renal stones for shock wave lithotripsy: part 1. J Urol 2001; 166:28-32. [PMID: 11435816] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/20/2023]
Abstract
PURPOSE We developed a real-time tracking system for renal stones that decreases the number of shock waves and treatment time of shock wave lithotripsy. MATERIALS AND METHODS Ultrasound images were analyzed to identify the renal stones. A computer software module for ultrasound image processing was developed to monitor stone location instantaneously. Another computer software module controlled generator movement in real time for tracking the stone. We used 13 ultrasound stone trajectories recorded from patients to test the system in vitro. Two tests were established to verify tracking system reliability. One test focused on improvement in the coincidence ratio, which denotes the matching extent of the stone within the effective focal area. The other test focused on improvement in the efficiency ratio, that is a decrease in the number of shocks for stone fragmentation. For each recorded stone trajectory 2 experiments were done under tracking and nontracking conditions. RESULTS The average coincidence and efficiency ratios plus or minus standard deviation were 79.6% +/- 9.8% and 45.0% +/- 12.7% without tracking, and 97.0% +/- 3.0% and 85.5 +/- 6.8% with tracking, respectively. All tests were statistically significant (paired t test p <0.01). CONCLUSIONS An ultrasound based real-time tracking system proved to be significantly helpful for in vitro lithotripsy. It appears that the tracking system may greatly decrease the number of shocks and treatment time for renal stones.
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Affiliation(s)
- C C Chang
- Department of Urology, ESWL Laboratory, National Cheng Kung University and Hospital, Tainan, Taiwan, Republic of China
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Chen ML, Kuo CL. A conserved sequence block in the murine and human T cell receptor Jalpha loci interacts with developmentally regulated nucleoprotein complexes in vitro and associates with GATA-3 and octamer-binding factors in vivo. Eur J Immunol 2001; 31:1696-705. [PMID: 11385613 DOI: 10.1002/1521-4141(200106)31:6<1696::aid-immu1696>3.0.co;2-n] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/08/2022]
Abstract
A highly conserved sequence block (CSB) located in the mouse and human T cell receptor (TCR) Jalpha loci is recognized by tissue-specific factors and up-regulates TCR alpha enhancer activity. In this study, the properties of CSB-interacting factors were further explored to decipher the function of this cis-acting element. Thymocytes corresponding to different developmental stages were found capable of forming differential CSB-nucleoprotein complexes. Pronounced changes in the CSB-complex-forming activity were observed during the transition from double-negative to double-positive thymocytes. Furthermore, we showed that transcription factors Oct-1, Oct-2 and GATA-3 interacted with CSB both in vitro, as evidenced by electrophoretic mobility shift assays, and in vivo, as demonstrated by chromatin immunoprecipitation assays in mouse thymus. Importantly, we also demonstrated that GATA-3 associated in vivo with TCR alpha enhancer, the activity of which is known to be required in regulating chromatin accessibility to the V(D)J recombinase. Thus, CSB may temporally regulate local chromatin structure and help to spread TCR alpha enhancer activity over the entire 70-kb Jalpha locus by forming developmentally regulated CSB-nucleoprotein complexes and by interacting with other cis-regulatory element-nucleoprotein complexes present within the TCR alpha / delta locus.
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Affiliation(s)
- M L Chen
- Institute of Biochemical Sciences, College of Science, National Taiwan University, Taipei, Taiwan, Republic of China
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Affiliation(s)
- C H Chen
- Division of Gastroenterology, Department of Internal Medicine, Changhua Show-Chwan Memorial Hospital, Taiwan, Republic of China
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Abstract
Aldehydes are known to inactivate cytochrome P450 in the reconstituted enzyme system containing NADPH and NADPH-cytochrome P450 reductase under aerobic conditions in a mechanism-based reaction involving heme adduct formation [Raner, G. M., Chiang, E. W. , Vaz, A. D. N., and Coon, M. J. (1997) Biochemistry 36, 4895-4902]. In the study presented here, artificial oxidants were used to examine the mechanism of aldehyde activation by purified P450 2B4 in the absence of the usual O(2)-reducing system, and the adducts that were formed were isolated and characterized. With hydrogen peroxide as the oxidant, 3-phenylpropionaldehyde gives an adduct with a mass corresponding to that of native heme modified by a phenylethyl group, presumably arising from the reaction of a peroxy-iron species with the aldehyde to give a peroxyhemiacetal, which upon deformylation yields the alkyl radical. NMR analysis indicated that the substitution is specifically at the gamma-meso position. In contrast, with m-chloroperbenzoic acid as the oxidant, an adduct is formed from 3-phenylpropionaldehyde with a mass that is consistent with the addition of a phenylpropionyl group, apparently arising by hydrogen abstraction from the aldehyde to give the carbonyl carbon radical. m-Chloroperbenzoic acid by itself forms a heme adduct with a mass corresponding to the addition of a chlorobenzoyloxy group apparently derived from homolytic oxygen-oxygen bond cleavage. These and other results with nonanal and 2-trans-nonenal support the concept that this versatile enzyme utilizes discrete oxidizing species in heme adduct formation from aldehydes.
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Affiliation(s)
- C L Kuo
- Department of Biological Chemistry, Medical School, The University of Michigan, Ann Arbor 48109-0606, USA
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Pang WW, Kuo CL, Huang HS, Wong E, Tang JC, Huang MH. Epidural catheter placement in the rabbit--a novel approach. Acta Anaesthesiol Sin 1999; 37:79-82. [PMID: 10410407] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 02/13/2023]
Abstract
BACKGROUND Using a pediatric epidural set and through caudal approach, we studied a relatively non-invasive technique for epidural percutaneous cannulation in rabbit for chronic laboratory investigations. METHODS Ten rabbits weighing over 3 kg were chosen and anesthetized with intravenous pentothal. A #19 pediatric Touhy needle and 23-gauge catheter were used for cannulation. Via the caudal approach, the epidural space could be located either by a "give" or with a technique of loss of resistance. Under fluoroscopy the catheter was tested with the injection of contrast medium for the confirmation of the proper position. The catheter was then tunneled under the skin and secured. The rabbits were kept in standard care for 4 weeks and then sacrificed by intraperitoneal pentothal overdose. A pathologist blinded to the study carefully examined the whole spine by laminectomy from cervical to coccyx and the findings were recorded. RESULTS With the injection of contrast medium, the final position of the catheter was validated by fluoroscopy in all rabbits. Two rabbits sustained immediate complications from the contrast medium and/or technique, of which one died shortly after the contrast medium injection and the other had weakness of the hind legs for a week. At sacrifice, all the catheters were found in good position. Two had hematoma associated with signs of trauma. One developed subcutaneous abscess. One had stitch infection of skin. CONCLUSIONS Percutaneous cannulation of epidural catheter is possible in the rabbit. Complications could be ameliorated by prudent approach in a skillful hand. It can be a reasonable model for the study of centrally administered medicines and their neurotoxicity.
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Affiliation(s)
- W W Pang
- Department of Anesthesia, Hsin Yun Ho General Hospital, Tao-Yuan, Taiwan, R.O.C
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Jiang Y, Kuo CL, Pernecky SJ, Coon MJ, Piper WN. Cytochrome P450 2E1 mRNA in the rat prostate: detection and quantitation by competitive reverse transcription and polymerase chain reaction. Mol Cell Probes 1998; 12:263-71. [PMID: 9778451 DOI: 10.1006/mcpr.1998.0177] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/22/2022]
Abstract
Cytochrome P450 2E1 plays a pivotal role in the metabolic activation of a wide variety of low molecular weight environmental toxicants and procarcinogens. In the present study, expression of the P450 2E1 gene in the rat prostate gland was quantitated by competitive reverse transcription and the polymerase chain reaction. To assess accurately the induction level of P450 2E1 mRNA in the prostate after pyridine treatment of rats, a recombinant standard RNA was generated that is homologous to the sequence of P450 2E1 mRNA except for an internal deletion of 100 bases. The data indicate that P450 2E1 mRNA is present in the prostate of untreated animals and is induced about four-fold by treatment with pyridine. The results suggest that exposure to certain environmental chemicals and procarcinogens may increase P450 2E1 levels in the prostate gland and thus could enhance formation of reactive, carcinogenic metabolites.
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Affiliation(s)
- Y Jiang
- Toxicology Program, Department of Environmental and Industrial Health, School of Public Health, The University of Michigan, Ann Arbor, MI 48109-2029, USA
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Kuo CL, La Du BN. Calcium binding by human and rabbit serum paraoxonases. Structural stability and enzymatic activity. Drug Metab Dispos 1998; 26:653-60. [PMID: 9660847] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/08/2023] Open
Abstract
Equilibrium dialysis and Scatchard plots were used to establish that human and rabbit paraoxonases both have two calcium binding sites. Independent-site and stepwise constant analyses were used to calculate a higher affinity site (Kd1) of 3.6 +/- 0.9 x 10(-7) M for human A paraoxonase, and 1.4 +/- 0.5 x 10(-8) M for rabbit paraoxonase, and a lower affinity site (Kd2) of 6.6 +/- 1.2 x 10(-6) M for human A paraoxonase, and 5.3 +/- 0.94 x 10(-6) M for rabbit paraoxonase. In both species, the higher affinity sites were found to be essential to maintain hydrolytic activity; complete removal of calcium led to irreversible inactivation. The lower affinity sites were required for catalytic activity, and their binding of calcium was reversible. Experimentally estimated values of Kd2 based on the concentration of calcium required to obtain half the maximum enzymatic activity were 3 microM for human A and B paraoxonases, and also in the order of 3 microM for rabbit paraoxonase, using three different substrates. Calcium was the only metal found that protects against denaturation and also confers hydrolytic activity with these two mammalian paraoxonases.
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Affiliation(s)
- C L Kuo
- Department of Environmental and Industrial Health, Toxicology Program, School of Public Health, The University of Michigan Medical School, Ann Arbor, MI 48109-0615, USA
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Abstract
Cytochrome P450 2E1 participates in the bioactivation of a wide variety of environmental and occupational pollutants. Such reactions may lead to the production of active carcinogenic metabolites. The presence of P450 2E1 in the testis and prostate has not yet been reported. In the present study, cytochrome P450 2E1 mRNA has been identified in the rat prostate and testis by reverse transcription PCR, southern blotting, and DNA sequencing. P450 2E1 protein from rat testis could be detected with immunoblot analysis, but was not detected in the prostate. The hydroxylation of p-nitrophenol, known to be mediated by P450 2E1, was demonstrated by HPLC measurement of product formation in microsomal fractions from the rat testis, but again not from prostate. Exposure of rats to pyridine resulted in a 2.9-fold increase of p-nitrophenol hydroxylation by testicular microsomes. Diethyldithiocarbamate, a selective mechanism-based inhibitor of P450 2E1, or a P450 2E1 monoclonal antibody, caused marked inhibition of testicular microsomal p-nitrophenol hydroxylase activity. These results indicate that cytochrome P450 2E1 is present in the rat testis, and that it is elevated by the treatment of the animals with pyridine. Thus, the presence and inducibility of cytochrome P450 2E1 in the testis may be of significance in the bioactivation of environmental chemicals to genotoxic metabolites.
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Affiliation(s)
- Y Jiang
- Department of Environmental and Industrial Health, School of Public Health, University of Michigan, Ann Arbor 48109-2029, USA
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Kuo CL, Chen ML, Wang K, Chou CK, Vernooij B, Seto D, Koop BF, Hood L. A conserved sequence block in murine and human T cell receptor (TCR) Jalpha region is a composite element that enhances TCR alpha enhancer activity and binds multiple nuclear factors. Proc Natl Acad Sci U S A 1998; 95:3839-44. [PMID: 9520454 PMCID: PMC19924 DOI: 10.1073/pnas.95.7.3839] [Citation(s) in RCA: 13] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/06/2023] Open
Abstract
A conserved sequence block (CSB) located in a noncoding region of the mouse and human TCR alpha/delta loci, showing six differences over 125 nucleotide positions (95% similar), was subjected to detailed analyses in this study. Transient transfection results showed that the CSB-containing element in conjunction with the TCR alpha enhancer up-regulated the alpha enhancer activity, whereas no enhancer activity was detected when CSB alone was assayed. In vitro occupancy analyses of CSB by nuclear factors reveal the existence of an unexpectedly intricate network of CSB-protein and protein-protein interactions. Lymphoid-specific as well as T-lineage-specific nuclear factors are involved to differentially form CSB-bound complexes in extracts of various tissues and cell lines. Liver was shown to contain factor(s) sequestering thymic CSB-binding factors. Furthermore, the putative binding sites for transcription factors known to be important for lymphoid-lineage development are present in CSB and are targeted by nuclear factors. On the basis of these results, we propose that the CSB element may play a role in shaping the chromatin structure by which the accessibility of TCR alpha/delta loci to the recombinase complex and/or to the transcriptional apparatus can be controlled.
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MESH Headings
- Animals
- Base Sequence
- Binding Sites/genetics
- Conserved Sequence
- Enhancer Elements, Genetic/genetics
- Enhancer Elements, Genetic/immunology
- Humans
- Mice
- Molecular Sequence Data
- Nuclear Proteins/immunology
- Receptors, Antigen, T-Cell, alpha-beta/genetics
- Receptors, Antigen, T-Cell, alpha-beta/immunology
- Receptors, Antigen, T-Cell, gamma-delta/genetics
- Receptors, Antigen, T-Cell, gamma-delta/immunology
- Sequence Analysis
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Affiliation(s)
- C L Kuo
- Institute of Biochemical Sciences, College of Science, National Taiwan University, Taipei, Taiwan, Republic of China.
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Kuo CL, Vaz AD, Coon MJ. Metabolic activation of trans-4-hydroxy-2-nonenal, a toxic product of membrane lipid peroxidation and inhibitor of P450 cytochromes. J Biol Chem 1997; 272:22611-6. [PMID: 9278417 DOI: 10.1074/jbc.272.36.22611] [Citation(s) in RCA: 18] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/05/2023] Open
Abstract
Lipid peroxidation in biological membranes is known to yield reactive aldehydes, of which trans-4-hydroxy-2-nonenal (HNE) is particularly cytotoxic. This laboratory previously reported that purified liver microsomal P450 cytochromes are directly inactivated to varying extents by HNE. We have now found a mechanism-based reaction in which P450s are inactivated by HNE in the presence of molecular oxygen, NADPH, and NADPH-cytochrome P450 reductase. The sensitivity of the various isozymes in the two pathways is different as follows: P450 2B4 and the orthologous 2B1 are inactivated to the greatest extent and 2C3, 1A2, 2E1, and 1A1 to a somewhat lesser extent by the pathway in which HNE undergoes metabolic activation. In contrast, 2B4 and 2B1 are insensitive to direct inactivation, and the reductase is unaffected by HNE by either route. Recent studies on the catalytic activities of the T302A mutant of P450 2B4 have shown that the rate of oxidation of a variety of xenobiotic aldehydes to carboxylic acids is decreased, but the rates of aldehyde deformylation and mechanism-based inactivation of the cytochrome are stimulated over those of the wild-type enzyme (Raner, G. M., Vaz, A. D. N., and Coon, M. J. (1997) Biochemistry 36, 4895-4902). Inactivation by those aldehydes apparently occurs by homolytic cleavage of a peroxyhemiacetal intermediate to yield formate and an alkyl radical that reacts with the heme. In sharp contrast, the rate of mechanism-based inactivation by HNE is decreased with the T302A mutant relative to that of the wild-type P450 2B4, and mass spectral analysis of the heme adduct formed shows that deformylation does not occur. We therefore propose that the metabolic activation of HNE involves formation of an acyl carbon radical that leads to the carboxylic acid or alternatively reacts with the heme.
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Affiliation(s)
- C L Kuo
- Department of Biological Chemistry, The University of Michigan Medical School, Ann Arbor, Michigan 48109-0606, USA
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Wang K, Gan L, Kuo CL, Hood L. A highly conserved apoptotic suppressor gene is located near the chicken T-cell receptor alpha chain constant region. Immunogenetics 1997; 46:376-82. [PMID: 9271627 DOI: 10.1007/s002510050291] [Citation(s) in RCA: 20] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/05/2023]
Abstract
A cosmid clone containing the chicken T-cell receptor alpha chain constant region (TCRAC) was sequenced. The cosmid contains the TCRAC gene, six putative joining gene segments (TCRAJ), and surprisingly, a chicken homologue for the human apoptotic suppressor gene, defender against cell death (DAD1). The DAD1 gene is 6.3 kilobases downstream of the TCRAC gene and has an inverted transcription orientation with respect to the TCRAC gene. The cDNA for the chicken DAD1 gene is 597 base pairs in length and encodes a highly conserved hydrophobic protein. The proximal location of DAD1 to the TCRAC locus has also been confirmed in both humans and mouse. The location of the DAD1 gene suggests that DAD1 may play an important role in T-cell related apoptotic activities.
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Affiliation(s)
- K Wang
- Department of Molecular Biotechnology, University of Washington, Box 357730, Seattle, WA 98195, USA
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Kuo CL, La Du BN. Comparison of purified human and rabbit serum paraoxonases. Drug Metab Dispos 1995; 23:935-44. [PMID: 8565784] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/31/2023] Open
Abstract
Rabbit serum paraoxonase (PON) activity was reported to be nearly 20 times greater than that found for humans and all other mammalian species tested, to date. However, 85% of the amino acid residues are identical in human and rabbit PONs, and the two purified PONs show similar substrate specificity patterns. Both are stimulated by phospholipids and have two asparagine-linked sugar chains. Both also have one intramolecular disulfide bond and one free sulfhydryl residue per molecule. Both require Ca2+ for stability and for catalytic activity. Zn2+ and Cd2+ also stabilize both PONs and prevent irreversible denaturation, but neither metal confers catalytic activity. Maximum specific activities for both esterases were approximately 2,000 units of arylesterase activity/mg protein. In contrast, rabbit PON is more stable than human PON to heat inactivation and sodium dodecyl sulfate-polyacrylamide gel electrophoresis treatment. Chelex 100 strips Ca2+ from human PON more easily, and EDTA is less inhibitory with rabbit PON. We conclude that human and rabbit PONs have very similar active centers, but the latter binds Ca2+ more tightly, is a more stable enzyme, and is maintained at 3- to 4-fold higher steady-state concentrations in serum than its human counterpart. PON activity depends on adequate Ca2+ being available; therefore, apparently much higher levels of PON activity in rabbits can be explained by the reduced Ca2+ concentrations present in the early assay methods.
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Affiliation(s)
- C L Kuo
- Department of Environmental and Industrial Health, School of Public Health, University of Michigan Medical School, Ann Arbor 48109-0572, USA
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