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Forero-Florez SC, Ball MAZ, Escobar-Díaz MC, Sanchez-de-Toledo J, Carretero J, Camprubí-Camprubí M. Percutaneous versus surgical closure of patent ductus arteriosus in low-weight premature infants: 10-year experience in a tertiary center. An Pediatr (Barc) 2024; 101:217-219. [PMID: 39218706 DOI: 10.1016/j.anpede.2024.06.008] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/13/2024] [Revised: 06/14/2024] [Accepted: 06/20/2024] [Indexed: 09/04/2024] Open
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Pandey S, Krause E, DeRose J, MacCrann N, Jain B, Crocce M, Blazek J, Choi A, Huang H, To C, Fang X, Elvin-Poole J, Prat J, Porredon A, Secco L, Rodriguez-Monroy M, Weaverdyck N, Park Y, Raveri M, Rozo E, Rykoff E, Bernstein G, Sánchez C, Jarvis M, Troxel M, Zacharegkas G, Chang C, Alarcon A, Alves O, Amon A, Andrade-Oliveira F, Baxter E, Bechtol K, Becker M, Camacho H, Campos A, Carnero Rosell A, Carrasco Kind M, Cawthon R, Chen R, Chintalapati P, Davis C, Di Valentino E, Diehl H, Dodelson S, Doux C, Drlica-Wagner A, Eckert K, Eifler T, Elsner F, Everett S, Farahi A, Ferté A, Fosalba P, Friedrich O, Gatti M, Giannini G, Gruen D, Gruendl R, Harrison I, Hartley W, Huff E, Huterer D, Kovacs A, Leget P, McCullough J, Muir J, Myles J, Navarro-Alsina A, Omori Y, Rollins R, Roodman A, Rosenfeld R, Sevilla-Noarbe I, Sheldon E, Shin T, Troja A, Tutusaus I, Varga T, Wechsler R, Yanny B, Yin B, Zhang Y, Zuntz J, Abbott T, Aguena M, Allam S, Annis J, Bacon D, Bertin E, Brooks D, Burke D, Carretero J, Conselice C, Costanzi M, da Costa L, Pereira M, De Vicente J, Dietrich J, Doel P, Evrard A, Ferrero I, Flaugher B, Frieman J, García-Bellido J, Gaztanaga E, Gerdes D, Giannantonio T, Gschwend J, Gutierrez G, Hinton S, Hollowood D, Honscheid K, James D, Jeltema T, Kuehn K, Kuropatkin N, Lahav O, Lima M, Lin H, Maia M, Marshall J, Melchior P, Menanteau F, Miller C, Miquel R, Mohr J, Morgan R, Palmese A, Paz-Chinchón F, Petravick D, Pieres A, Plazas Malagón A, Sanchez E, Scarpine V, Serrano S, Smith M, Soares-Santos M, Suchyta E, Tarle G, Thomas D, Weller J. Dark Energy Survey year 3 results: Constraints on cosmological parameters and galaxy-bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.106.043520] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Abbott T, Aguena M, Alarcon A, Allam S, Alves O, Amon A, Andrade-Oliveira F, Annis J, Avila S, Bacon D, Baxter E, Bechtol K, Becker M, Bernstein G, Bhargava S, Birrer S, Blazek J, Brandao-Souza A, Bridle S, Brooks D, Buckley-Geer E, Burke D, Camacho H, Campos A, Carnero Rosell A, Carrasco Kind M, Carretero J, Castander F, Cawthon R, Chang C, Chen A, Chen R, Choi A, Conselice C, Cordero J, Costanzi M, Crocce M, da Costa L, da Silva Pereira M, Davis C, Davis T, De Vicente J, DeRose J, Desai S, Di Valentino E, Diehl H, Dietrich J, Dodelson S, Doel P, Doux C, Drlica-Wagner A, Eckert K, Eifler T, Elsner F, Elvin-Poole J, Everett S, Evrard A, Fang X, Farahi A, Fernandez E, Ferrero I, Ferté A, Fosalba P, Friedrich O, Frieman J, García-Bellido J, Gatti M, Gaztanaga E, Gerdes D, Giannantonio T, Giannini G, Gruen D, Gruendl R, Gschwend J, Gutierrez G, Harrison I, Hartley W, Herner K, Hinton S, Hollowood D, Honscheid K, Hoyle B, Huff E, Huterer D, Jain B, James D, Jarvis M, Jeffrey N, Jeltema T, Kovacs A, Krause E, Kron R, Kuehn K, Kuropatkin N, Lahav O, Leget PF, Lemos P, Liddle A, Lidman C, Lima M, Lin H, MacCrann N, Maia M, Marshall J, Martini P, McCullough J, Melchior P, Mena-Fernández J, Menanteau F, Miquel R, Mohr J, Morgan R, Muir J, Myles J, Nadathur S, Navarro-Alsina A, Nichol R, Ogando R, Omori Y, Palmese A, Pandey S, Park Y, Paz-Chinchón F, Petravick D, Pieres A, Plazas Malagón A, Porredon A, Prat J, Raveri M, Rodriguez-Monroy M, Rollins R, Romer A, Roodman A, Rosenfeld R, Ross A, Rykoff E, Samuroff S, Sánchez C, Sanchez E, Sanchez J, Sanchez Cid D, Scarpine V, Schubnell M, Scolnic D, Secco L, Serrano S, Sevilla-Noarbe I, Sheldon E, Shin T, Smith M, Soares-Santos M, Suchyta E, Swanson M, Tabbutt M, Tarle G, Thomas D, To C, Troja A, Troxel M, Tucker D, Tutusaus I, Varga T, Walker A, Weaverdyck N, Wechsler R, Weller J, Yanny B, Yin B, Zhang Y, Zuntz J. Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.105.023520] [Citation(s) in RCA: 106] [Impact Index Per Article: 53.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Amon A, Gruen D, Troxel M, MacCrann N, Dodelson S, Choi A, Doux C, Secco L, Samuroff S, Krause E, Cordero J, Myles J, DeRose J, Wechsler R, Gatti M, Navarro-Alsina A, Bernstein G, Jain B, Blazek J, Alarcon A, Ferté A, Lemos P, Raveri M, Campos A, Prat J, Sánchez C, Jarvis M, Alves O, Andrade-Oliveira F, Baxter E, Bechtol K, Becker M, Bridle S, Camacho H, Carnero Rosell A, Carrasco Kind M, Cawthon R, Chang C, Chen R, Chintalapati P, Crocce M, Davis C, Diehl H, Drlica-Wagner A, Eckert K, Eifler T, Elvin-Poole J, Everett S, Fang X, Fosalba P, Friedrich O, Gaztanaga E, Giannini G, Gruendl R, Harrison I, Hartley W, Herner K, Huang H, Huff E, Huterer D, Kuropatkin N, Leget P, Liddle A, McCullough J, Muir J, Pandey S, Park Y, Porredon A, Refregier A, Rollins R, Roodman A, Rosenfeld R, Ross A, Rykoff E, Sanchez J, Sevilla-Noarbe I, Sheldon E, Shin T, Troja A, Tutusaus I, Tutusaus I, Varga T, Weaverdyck N, Yanny B, Yin B, Zhang Y, Zuntz J, Aguena M, Allam S, Annis J, Bacon D, Bertin E, Bhargava S, Brooks D, Buckley-Geer E, Burke D, Carretero J, Costanzi M, da Costa L, Pereira M, De Vicente J, Desai S, Dietrich J, Doel P, Ferrero I, Flaugher B, Frieman J, García-Bellido J, Gaztanaga E, Gerdes D, Giannantonio T, Gschwend J, Gutierrez G, Hinton S, Hollowood D, Honscheid K, Hoyle B, James D, Kron R, Kuehn K, Lahav O, Lima M, Lin H, Maia M, Marshall J, Martini P, Melchior P, Menanteau F, Miquel R, Mohr J, Morgan R, Ogando R, Palmese A, Paz-Chinchón F, Petravick D, Pieres A, Romer A, Sanchez E, Scarpine V, Schubnell M, Serrano S, Smith M, Soares-Santos M, Tarle G, Thomas D, To C, Weller J. Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.105.023514] [Citation(s) in RCA: 42] [Impact Index Per Article: 21.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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To C, Krause E, Rozo E, Wu H, Gruen D, Wechsler RH, Eifler TF, Rykoff ES, Costanzi M, Becker MR, Bernstein GM, Blazek J, Bocquet S, Bridle SL, Cawthon R, Choi A, Crocce M, Davis C, DeRose J, Drlica-Wagner A, Elvin-Poole J, Fang X, Farahi A, Friedrich O, Gatti M, Gaztanaga E, Giannantonio T, Hartley WG, Hoyle B, Jarvis M, MacCrann N, McClintock T, Miranda V, Pereira MES, Park Y, Porredon A, Prat J, Rau MM, Ross AJ, Samuroff S, Sánchez C, Sevilla-Noarbe I, Sheldon E, Troxel MA, Varga TN, Vielzeuf P, Zhang Y, Zuntz J, Abbott TMC, Aguena M, Amon A, Annis J, Avila S, Bertin E, Bhargava S, Brooks D, Burke DL, Carnero Rosell A, Carrasco Kind M, Carretero J, Chang C, Conselice C, da Costa LN, Davis TM, Desai S, Diehl HT, Dietrich JP, Everett S, Evrard AE, Ferrero I, Flaugher B, Fosalba P, Frieman J, García-Bellido J, Gruendl RA, Gutierrez G, Hinton SR, Hollowood DL, Honscheid K, Huterer D, James DJ, Jeltema T, Kron R, Kuehn K, Kuropatkin N, Lima M, Maia MAG, Marshall JL, Menanteau F, Miquel R, Morgan R, Muir J, Myles J, Palmese A, Paz-Chinchón F, Plazas AA, Romer AK, Roodman A, Sanchez E, Santiago B, Scarpine V, Serrano S, Smith M, Suchyta E, Swanson MEC, Tarle G, Thomas D, Tucker DL, Weller J, Wester W, Wilkinson RD. Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations. PHYSICAL REVIEW LETTERS 2021; 126:141301. [PMID: 33891448 DOI: 10.1103/physrevlett.126.141301] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/06/2020] [Revised: 01/07/2021] [Accepted: 02/23/2021] [Indexed: 06/12/2023]
Abstract
We present the first joint analysis of cluster abundances and auto or cross-correlations of three cosmic tracer fields: galaxy density, weak gravitational lensing shear, and cluster density split by optical richness. From a joint analysis (4×2pt+N) of cluster abundances, three cluster cross-correlations, and the auto correlations of the galaxy density measured from the first year data of the Dark Energy Survey, we obtain Ω_{m}=0.305_{-0.038}^{+0.055} and σ_{8}=0.783_{-0.054}^{+0.064}. This result is consistent with constraints from the DES-Y1 galaxy clustering and weak lensing two-point correlation functions for the flat νΛCDM model. Consequently, we combine cluster abundances and all two-point correlations from across all three cosmic tracer fields (6×2pt+N) and find improved constraints on cosmological parameters as well as on the cluster observable-mass scaling relation. This analysis is an important advance in both optical cluster cosmology and multiprobe analyses of upcoming wide imaging surveys.
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Garcia-Sanchez J, Benet M, Cordon L, Piqueras M, Garde-Noguera J, de Julian M, Gonzalez-Castillo L, Lorente D, Piera N, Gomez-Soler M, Ruiz V, Carretero J, Sanchez-Hernandez A, Juan-Vidal O, Lahoz A. 165P Baseline circulating myeloid-derived suppressor cells correlate with neutrophil-to-lymphocyte ratio and overall survival in advanced non-small cell lung cancer patients treated with immune checkpoint inhibitors. J Thorac Oncol 2021. [DOI: 10.1016/s1556-0864(21)02007-4] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/21/2022]
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Nadler EO, Drlica-Wagner A, Bechtol K, Mau S, Wechsler RH, Gluscevic V, Boddy K, Pace AB, Li TS, McNanna M, Riley AH, García-Bellido J, Mao YY, Green G, Burke DL, Peter A, Jain B, Abbott TMC, Aguena M, Allam S, Annis J, Avila S, Brooks D, Carrasco Kind M, Carretero J, Costanzi M, da Costa LN, De Vicente J, Desai S, Diehl HT, Doel P, Everett S, Evrard AE, Flaugher B, Frieman J, Gerdes DW, Gruen D, Gruendl RA, Gschwend J, Gutierrez G, Hinton SR, Honscheid K, Huterer D, James DJ, Krause E, Kuehn K, Kuropatkin N, Lahav O, Maia MAG, Marshall JL, Menanteau F, Miquel R, Palmese A, Paz-Chinchón F, Plazas AA, Romer AK, Sanchez E, Scarpine V, Serrano S, Sevilla-Noarbe I, Smith M, Soares-Santos M, Suchyta E, Swanson MEC, Tarle G, Tucker DL, Walker AR, Wester W. Constraints on Dark Matter Properties from Observations of Milky Way Satellite Galaxies. PHYSICAL REVIEW LETTERS 2021; 126:091101. [PMID: 33750144 DOI: 10.1103/physrevlett.126.091101] [Citation(s) in RCA: 6] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/30/2020] [Revised: 12/12/2020] [Accepted: 01/27/2021] [Indexed: 06/12/2023]
Abstract
We perform a comprehensive study of Milky Way (MW) satellite galaxies to constrain the fundamental properties of dark matter (DM). This analysis fully incorporates inhomogeneities in the spatial distribution and detectability of MW satellites and marginalizes over uncertainties in the mapping between galaxies and DM halos, the properties of the MW system, and the disruption of subhalos by the MW disk. Our results are consistent with the cold, collisionless DM paradigm and yield the strongest cosmological constraints to date on particle models of warm, interacting, and fuzzy dark matter. At 95% confidence, we report limits on (i) the mass of thermal relic warm DM, m_{WDM}>6.5 keV (free-streaming length, λ_{fs}≲10h^{-1} kpc), (ii) the velocity-independent DM-proton scattering cross section, σ_{0}<8.8×10^{-29} cm^{2} for a 100 MeV DM particle mass [DM-proton coupling, c_{p}≲(0.3 GeV)^{-2}], and (iii) the mass of fuzzy DM, m_{ϕ}>2.9×10^{-21} eV (de Broglie wavelength, λ_{dB}≲0.5 kpc). These constraints are complementary to other observational and laboratory constraints on DM properties.
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Costanzi M, Saro A, Bocquet S, Abbott T, Aguena M, Allam S, Amara A, Annis J, Avila S, Bacon D, Benson B, Bhargava S, Brooks D, Buckley-Geer E, Burke D, Carnero Rosell A, Carrasco Kind M, Carretero J, Choi A, da Costa L, Pereira M, De Vicente J, Desai S, Diehl H, Dietrich J, Doel P, Eifler T, Everett S, Ferrero I, Ferté A, Flaugher B, Fosalba P, Frieman J, García-Bellido J, Gaztanaga E, Gerdes D, Giannantonio T, Giles P, Grandis S, Gruen D, Gruendl R, Gupta N, Gutierrez G, Hartley W, Hinton S, Hollowood D, Honscheid K, James D, Jeltema T, Krause E, Kuehn K, Kuropatkin N, Lahav O, Lima M, MacCrann N, Maia M, Marshall J, Menanteau F, Miquel R, Mohr J, Morgan R, Myles J, Ogando R, Palmese A, Paz-Chinchón F, Plazas A, Rapetti D, Reichardt C, Romer A, Roodman A, Ruppin F, Salvati L, Samuroff S, Sanchez E, Scarpine V, Serrano S, Sevilla-Noarbe I, Singh P, Smith M, Soares-Santos M, Stark A, Suchyta E, Swanson M, Tarle G, Thomas D, To C, Tucker D, Varga T, Wechsler R, Zhang Z. Cosmological constraints from DES Y1 cluster abundances and SPT multiwavelength data. Int J Clin Exp Med 2021. [DOI: 10.1103/physrevd.103.043522] [Citation(s) in RCA: 17] [Impact Index Per Article: 5.7] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Muir J, Baxter E, Miranda V, Doux C, Ferté A, Leonard C, Huterer D, Jain B, Lemos P, Raveri M, Nadathur S, Campos A, Chen A, Dodelson S, Elvin-Poole J, Lee S, Secco L, Troxel M, Weaverdyck N, Zuntz J, Brout D, Choi A, Crocce M, Davis T, Gruen D, Krause E, Lidman C, MacCrann N, Möller A, Prat J, Ross A, Sako M, Samuroff S, Sánchez C, Scolnic D, Zhang B, Abbott T, Aguena M, Allam S, Annis J, Avila S, Bacon D, Bertin E, Bhargava S, Bridle S, Brooks D, Burke D, Carnero Rosell A, Carrasco Kind M, Carretero J, Cawthon R, Costanzi M, da Costa L, Pereira M, Desai S, Diehl H, Dietrich J, Doel P, Estrada J, Everett S, Evrard A, Ferrero I, Flaugher B, Frieman J, García-Bellido J, Giannantonio T, Gruendl R, Gschwend J, Gutierrez G, Hinton S, Hollowood D, Honscheid K, Hoyle B, James D, Jeltema T, Kuehn K, Kuropatkin N, Lahav O, Lima M, Maia M, Menanteau F, Miquel R, Morgan R, Myles J, Palmese A, Paz-Chinchón F, Plazas A, Romer A, Roodman A, Sanchez E, Scarpine V, Serrano S, Sevilla-Noarbe I, Smith M, Suchyta E, Swanson M, Tarle G, Thomas D, To C, Tucker D, Varga T, Weller J, Wilkinson R. DES Y1 results: Splitting growth and geometry to test
ΛCDM. Int J Clin Exp Med 2021. [DOI: 10.1103/physrevd.103.023528] [Citation(s) in RCA: 10] [Impact Index Per Article: 3.3] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Pros E, Saigi M, Alameda D, Gomez-Mariano G, Martinez-Delgado B, Alburquerque-Bejar JJ, Carretero J, Tonda R, Esteve-Codina A, Catala I, Palmero R, Jove M, Lazaro C, Patiño-Garcia A, Gil-Bazo I, Verdura S, Teulé A, Torres-Lanzas J, Sidransky D, Reguart N, Pio R, Juan-Vidal O, Nadal E, Felip E, Montuenga LM, Sanchez-Cespedes M. Genome-wide profiling of non-smoking-related lung cancer cells reveals common RB1 rearrangements associated with histopathologic transformation in EGFR-mutant tumors. Ann Oncol 2021; 31:274-282. [PMID: 31959344 DOI: 10.1016/j.annonc.2019.09.001] [Citation(s) in RCA: 23] [Impact Index Per Article: 7.7] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/05/2019] [Revised: 09/25/2019] [Accepted: 09/26/2019] [Indexed: 10/25/2022] Open
Abstract
BACKGROUND The etiology and the molecular basis of lung adenocarcinomas (LuADs) in nonsmokers are currently unknown. Furthermore, the scarcity of available primary cultures continues to hamper our biological understanding of non-smoking-related lung adenocarcinomas (NSK-LuADs). PATIENTS AND METHODS We established patient-derived cancer cell (PDC) cultures from metastatic NSK-LuADs, including two pairs of matched EGFR-mutant PDCs before and after resistance to tyrosine kinase inhibitors (TKIs), and then performed whole-exome and RNA sequencing to delineate their genomic architecture. For validation, we analyzed independent cohorts of primary LuADs. RESULTS In addition to known non-smoker-associated alterations (e.g. RET, ALK, EGFR, and ERBB2), we discovered novel fusions and recurrently mutated genes, including ATF7IP, a regulator of gene expression, that was inactivated in 5% of primary LuAD cases. We also found germline mutations at dominant familiar-cancer genes, highlighting the importance of genetic predisposition in the origin of a subset of NSK-LuADs. Furthermore, there was an over-representation of inactivating alterations at RB1, mostly through complex intragenic rearrangements, in treatment-naive EGFR-mutant LuADs. Three EGFR-mutant and one EGFR-wild-type tumors acquired resistance to EGFR-TKIs and chemotherapy, respectively, and histology on re-biopsies revealed the development of small-cell lung cancer/squamous cell carcinoma (SCLC/LuSCC) transformation. These features were consistent with RB1 inactivation and acquired EGFR-T790M mutation or FGFR3-TACC3 fusion in EGFR-mutant tumors. CONCLUSIONS We found recurrent alterations in LuADs that deserve further exploration. Our work also demonstrates that a subset of NSK-LuADs arises within cancer-predisposition syndromes. The preferential occurrence of RB1 inactivation, via complex rearrangements, found in EGFR-mutant tumors appears to favor SCLC/LuSCC transformation under growth-inhibition pressures. Thus RB1 inactivation may predict the risk of LuAD transformation to a more aggressive type of lung cancer, and may need to be considered as a part of the clinical management of NSK-LuADs patients.
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Abbott T, Aguena M, Alarcon A, Allam S, Allen S, Annis J, Avila S, Bacon D, Bechtol K, Bermeo A, Bernstein G, Bertin E, Bhargava S, Bocquet S, Brooks D, Brout D, Buckley-Geer E, Burke D, Carnero Rosell A, Carrasco Kind M, Carretero J, Castander F, Cawthon R, Chang C, Chen X, Choi A, Costanzi M, Crocce M, da Costa L, Davis T, De Vicente J, DeRose J, Desai S, Diehl H, Dietrich J, Dodelson S, Doel P, Drlica-Wagner A, Eckert K, Eifler T, Elvin-Poole J, Estrada J, Everett S, Evrard A, Farahi A, Ferrero I, Flaugher B, Fosalba P, Frieman J, García-Bellido J, Gatti M, Gaztanaga E, Gerdes D, Giannantonio T, Giles P, Grandis S, Gruen D, Gruendl R, Gschwend J, Gutierrez G, Hartley W, Hinton S, Hollowood D, Honscheid K, Hoyle B, Huterer D, James D, Jarvis M, Jeltema T, Johnson M, Johnson M, Kent S, Krause E, Kron R, Kuehn K, Kuropatkin N, Lahav O, Li T, Lidman C, Lima M, Lin H, MacCrann N, Maia M, Mantz A, Marshall J, Martini P, Mayers J, Melchior P, Mena-Fernández J, Menanteau F, Miquel R, Mohr J, Nichol R, Nord B, Ogando R, Palmese A, Paz-Chinchón F, Plazas A, Prat J, Rau M, Romer A, Roodman A, Rooney P, Rozo E, Rykoff E, Sako M, Samuroff S, Sánchez C, Sanchez E, Saro A, Scarpine V, Schubnell M, Scolnic D, Serrano S, Sevilla-Noarbe I, Sheldon E, Smith J, Smith M, Suchyta E, Swanson M, Tarle G, Thomas D, To C, Troxel M, Tucker D, Varga T, von der Linden A, Walker A, Wechsler R, Weller J, Wilkinson R, Wu H, Yanny B, Zhang Y, Zhang Z, Zuntz J. Dark Energy Survey Year 1 Results: Cosmological constraints from cluster abundances and weak lensing. Int J Clin Exp Med 2020. [DOI: 10.1103/physrevd.102.023509] [Citation(s) in RCA: 98] [Impact Index Per Article: 24.5] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Kacprzak T, Herbel J, Nicola A, Sgier R, Tarsitano F, Bruderer C, Amara A, Refregier A, Bridle S, Drlica-Wagner A, Gruen D, Hartley W, Hoyle B, Secco L, Zuntz J, Annis J, Avila S, Bertin E, Brooks D, Buckley-Geer E, Carnero Rosell A, Carrasco Kind M, Carretero J, da Costa L, De Vicente J, Desai S, Diehl H, Doel P, García-Bellido J, Gaztanaga E, Gruendl R, Gschwend J, Gutierrez G, Hollowood D, Honscheid K, James D, Jarvis M, Lima M, Maia M, Marshall J, Melchior P, Menanteau F, Miquel R, Paz-Chinchón F, Plazas A, Sanchez E, Scarpine V, Serrano S, Sevilla-Noarbe I, Smith M, Suchyta E, Swanson M, Tarle G, Vikram V, Weller J. Monte Carlo control loops for cosmic shear cosmology with DES Year 1 data. Int J Clin Exp Med 2020. [DOI: 10.1103/physrevd.101.082003] [Citation(s) in RCA: 8] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Ammazzalorso S, Gruen D, Regis M, Camera S, Ando S, Fornengo N, Bechtol K, Bridle SL, Choi A, Eifler TF, Gatti M, MacCrann N, Omori Y, Samuroff S, Sheldon E, Troxel MA, Zuntz J, Carrasco Kind M, Annis J, Avila S, Bertin E, Brooks D, Burke DL, Carnero Rosell A, Carretero J, Castander FJ, Costanzi M, da Costa LN, De Vicente J, Desai S, Diehl HT, Dietrich JP, Doel P, Everett S, Flaugher B, Fosalba P, García-Bellido J, Gaztanaga E, Gerdes DW, Giannantonio T, Goldstein DA, Gruendl RA, Gutierrez G, Hollowood DL, Honscheid K, James DJ, Jarvis M, Jeltema T, Kent S, Kuropatkin N, Lahav O, Li TS, Lima M, Maia MAG, Marshall JL, Melchior P, Menanteau F, Miquel R, Ogando RLC, Palmese A, Plazas AA, Romer AK, Roodman A, Rykoff ES, Sánchez C, Sanchez E, Scarpine V, Serrano S, Sevilla-Noarbe I, Smith M, Soares-Santos M, Sobreira F, Suchyta E, Swanson MEC, Tarle G, Thomas D, Vikram V, Zhang Y. Detection of Cross-Correlation between Gravitational Lensing and γ Rays. PHYSICAL REVIEW LETTERS 2020; 124:101102. [PMID: 32216401 DOI: 10.1103/physrevlett.124.101102] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/22/2019] [Revised: 12/14/2019] [Accepted: 01/13/2020] [Indexed: 06/10/2023]
Abstract
In recent years, many γ-ray sources have been identified, yet the unresolved component hosts valuable information on the faintest emission. In order to extract it, a cross-correlation with gravitational tracers of matter in the Universe has been shown to be a promising tool. We report here the first identification of a cross-correlation signal between γ rays and the distribution of mass in the Universe probed by weak gravitational lensing. We use data from the Dark Energy Survey Y1 weak lensing data and the Fermi Large Area Telescope 9-yr γ-ray data, obtaining a signal-to-noise ratio of 5.3. The signal is mostly localized at small angular scales and high γ-ray energies, with a hint of correlation at extended separation. Blazar emission is likely the origin of the small-scale effect. We investigate implications of the large-scale component in terms of astrophysical sources and particle dark matter emission.
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Raghunathan S, Patil S, Baxter E, Benson BA, Bleem LE, Crawford TM, Holder GP, McClintock T, Reichardt CL, Varga TN, Whitehorn N, Ade PAR, Allam S, Anderson AJ, Austermann JE, Avila S, Avva JS, Bacon D, Beall JA, Bender AN, Bianchini F, Bocquet S, Brooks D, Burke DL, Carlstrom JE, Carretero J, Castander FJ, Chang CL, Chiang HC, Citron R, Costanzi M, Crites AT, da Costa LN, Desai S, Diehl HT, Dietrich JP, Dobbs MA, Doel P, Everett S, Evrard AE, Feng C, Flaugher B, Fosalba P, Frieman J, Gallicchio J, García-Bellido J, Gaztanaga E, George EM, Giannantonio T, Gilbert A, Gruendl RA, Gschwend J, Gupta N, Gutierrez G, de Haan T, Halverson NW, Harrington N, Henning JW, Hilton GC, Hollowood DL, Holzapfel WL, Honscheid K, Hrubes JD, Huang N, Hubmayr J, Irwin KD, Jeltema T, Kind MC, Knox L, Kuropatkin N, Lahav O, Lee AT, Li D, Lima M, Lowitz A, Maia MAG, Marshall JL, McMahon JJ, Melchior P, Menanteau F, Meyer SS, Miquel R, Mocanu LM, Mohr JJ, Montgomery J, Moran CC, Nadolski A, Natoli T, Nibarger JP, Noble G, Novosad V, Ogando RLC, Padin S, Plazas AA, Pryke C, Rapetti D, Romer AK, Roodman A, Rosell AC, Rozo E, Ruhl JE, Rykoff ES, Saliwanchik BR, Sanchez E, Sayre JT, Scarpine V, Schaffer KK, Schubnell M, Serrano S, Sevilla-Noarbe I, Sievers C, Smecher G, Smith M, Soares-Santos M, Stark AA, Story KT, Suchyta E, Swanson MEC, Tarle G, Tucker C, Vanderlinde K, Veach T, De Vicente J, Vieira JD, Vikram V, Wang G, Wu WLK, Yefremenko V, Zhang Y. Detection of CMB-Cluster Lensing using Polarization Data from SPTpol. PHYSICAL REVIEW LETTERS 2019; 123:181301. [PMID: 31763885 DOI: 10.1103/physrevlett.123.181301] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/30/2019] [Indexed: 06/10/2023]
Abstract
We report the first detection of gravitational lensing due to galaxy clusters using only the polarization of the cosmic microwave background (CMB). The lensing signal is obtained using a new estimator that extracts the lensing dipole signature from stacked images formed by rotating the cluster-centered Stokes QU map cutouts along the direction of the locally measured background CMB polarization gradient. Using data from the SPTpol 500 deg^{2} survey at the locations of roughly 18 000 clusters with richness λ≥10 from the Dark Energy Survey (DES) Year-3 full galaxy cluster catalog, we detect lensing at 4.8σ. The mean stacked mass of the selected sample is found to be (1.43±0.40)×10^{14}M_{⊙} which is in good agreement with optical weak lensing based estimates using DES data and CMB-lensing based estimates using SPTpol temperature data. This measurement is a key first step for cluster cosmology with future low-noise CMB surveys, like CMB-S4, for which CMB polarization will be the primary channel for cluster lensing measurements.
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Pandey S, Baxter E, Xu Z, Orlowski-Scherer J, Zhu N, Lidz A, Aguirre J, DeRose J, Devlin M, Hill J, Jain B, Sheth R, Avila S, Bertin E, Brooks D, Buckley-Geer E, Carnero Rosell A, Carrasco Kind M, Carretero J, Castander F, Cawthon R, da Costa L, De Vicente J, Desai S, Diehl H, Dietrich J, Doel P, Evrard A, Flaugher B, Fosalba P, Frieman J, García-Bellido J, Gerdes D, Giannantonio T, Gruendl R, Gschwend J, Hartley W, Hollowood D, James D, Krause E, Kuehn K, Kuropatkin N, Maia M, Marshall J, Melchior P, Menanteau F, Miquel R, Plazas A, Roodman A, Sanchez E, Serrano S, Sevilla-Noarbe I, Smith M, Soares-Santos M, Sobreira F, Suchyta E, Swanson M, Tarle G, Wechsler R. Constraints on the redshift evolution of astrophysical feedback with Sunyaev-Zel’dovich effect cross-correlations. Int J Clin Exp Med 2019. [DOI: 10.1103/physrevd.100.063519] [Citation(s) in RCA: 20] [Impact Index Per Article: 4.0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Omori Y, Baxter E, Chang C, Kirk D, Alarcon A, Bernstein G, Bleem L, Cawthon R, Choi A, Chown R, Crawford T, Davis C, De Vicente J, DeRose J, Dodelson S, Eifler T, Fosalba P, Friedrich O, Gatti M, Gaztanaga E, Giannantonio T, Gruen D, Hartley W, Holder G, Hoyle B, Huterer D, Jain B, Jarvis M, Krause E, MacCrann N, Miquel R, Prat J, Rau M, Reichardt C, Rozo E, Samuroff S, Sánchez C, Secco L, Sheldon E, Simard G, Troxel M, Vielzeuf P, Wechsler R, Zuntz J, Abbott T, Abdalla F, Allam S, Annis J, Avila S, Aylor K, Benson B, Bertin E, Bridle S, Brooks D, Burke D, Carlstrom J, Carnero Rosell A, Carrasco Kind M, Carretero J, Castander F, Chang C, Cho HM, Crites A, Crocce M, Cunha C, da Costa L, de Haan T, Desai S, Diehl H, Dietrich J, Dobbs M, Everett W, Fernandez E, Flaugher B, Frieman J, García-Bellido J, George E, Gruendl R, Gutierrez G, Halverson N, Harrington N, Hollowood D, Honscheid K, Holzapfel W, Hou Z, Hrubes J, James D, Jeltema T, Kuehn K, Kuropatkin N, Lima M, Lin H, Lee A, Leitch E, Luong-Van D, Maia M, Manzotti A, Marrone D, Marshall J, Martini P, McMahon J, Melchior P, Menanteau F, Meyer S, Mocanu L, Mohr J, Natoli T, Ogando R, Padin S, Plazas A, Pryke C, Romer A, Roodman A, Ruhl J, Rykoff E, Sanchez E, Scarpine V, Schaffer K, Schindler R, Sevilla-Noarbe I, Shirokoff E, Smith M, Smith R, Soares-Santos M, Sobreira F, Staniszewski Z, Stark A, Story K, Suchyta E, Swanson M, Tarle G, Thomas D, Vanderlinde K, Vieira J, Vikram V, Walker A, Weller J, Williamson R, Wu W, Zahn O. Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope
+Planck
CMB weak lensing. Int J Clin Exp Med 2019. [DOI: 10.1103/physrevd.100.043517] [Citation(s) in RCA: 12] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Abbott TMC, Alarcon A, Allam S, Andersen P, Andrade-Oliveira F, Annis J, Asorey J, Avila S, Bacon D, Banik N, Bassett BA, Baxter E, Bechtol K, Becker MR, Bernstein GM, Bertin E, Blazek J, Bridle SL, Brooks D, Brout D, Burke DL, Calcino J, Camacho H, Campos A, Carnero Rosell A, Carollo D, Carrasco Kind M, Carretero J, Castander FJ, Cawthon R, Challis P, Chan KC, Chang C, Childress M, Crocce M, Cunha CE, D'Andrea CB, da Costa LN, Davis C, Davis TM, De Vicente J, DePoy DL, DeRose J, Desai S, Diehl HT, Dietrich JP, Dodelson S, Doel P, Drlica-Wagner A, Eifler TF, Elvin-Poole J, Estrada J, Evrard AE, Fernandez E, Flaugher B, Foley RJ, Fosalba P, Frieman J, Galbany L, García-Bellido J, Gatti M, Gaztanaga E, Gerdes DW, Giannantonio T, Glazebrook K, Goldstein DA, Gruen D, Gruendl RA, Gschwend J, Gutierrez G, Hartley WG, Hinton SR, Hollowood DL, Honscheid K, Hoormann JK, Hoyle B, Huterer D, Jain B, James DJ, Jarvis M, Jeltema T, Kasai E, Kent S, Kessler R, Kim AG, Kokron N, Krause E, Kron R, Kuehn K, Kuropatkin N, Lahav O, Lasker J, Lemos P, Lewis GF, Li TS, Lidman C, Lima M, Lin H, Macaulay E, MacCrann N, Maia MAG, March M, Marriner J, Marshall JL, Martini P, McMahon RG, Melchior P, Menanteau F, Miquel R, Mohr JJ, Morganson E, Muir J, Möller A, Neilsen E, Nichol RC, Nord B, Ogando RLC, Palmese A, Pan YC, Peiris HV, Percival WJ, Plazas AA, Porredon A, Prat J, Romer AK, Roodman A, Rosenfeld R, Ross AJ, Rykoff ES, Samuroff S, Sánchez C, Sanchez E, Scarpine V, Schindler R, Schubnell M, Scolnic D, Secco LF, Serrano S, Sevilla-Noarbe I, Sharp R, Sheldon E, Smith M, Soares-Santos M, Sobreira F, Sommer NE, Swann E, Swanson MEC, Tarle G, Thomas D, Thomas RC, Troxel MA, Tucker BE, Uddin SA, Vielzeuf P, Walker AR, Wang M, Weaverdyck N, Wechsler RH, Weller J, Yanny B, Zhang B, Zhang Y, Zuntz J. Cosmological Constraints from Multiple Probes in the Dark Energy Survey. PHYSICAL REVIEW LETTERS 2019; 122:171301. [PMID: 31107093 DOI: 10.1103/physrevlett.122.171301] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/08/2018] [Revised: 02/19/2019] [Indexed: 06/09/2023]
Abstract
The combination of multiple observational probes has long been advocated as a powerful technique to constrain cosmological parameters, in particular dark energy. The Dark Energy Survey has measured 207 spectroscopically confirmed type Ia supernova light curves, the baryon acoustic oscillation feature, weak gravitational lensing, and galaxy clustering. Here we present combined results from these probes, deriving constraints on the equation of state, w, of dark energy and its energy density in the Universe. Independently of other experiments, such as those that measure the cosmic microwave background, the probes from this single photometric survey rule out a Universe with no dark energy, finding w=-0.80_{-0.11}^{+0.09}. The geometry is shown to be consistent with a spatially flat Universe, and we obtain a constraint on the baryon density of Ω_{b}=0.069_{-0.012}^{+0.009} that is independent of early Universe measurements. These results demonstrate the potential power of large multiprobe photometric surveys and pave the way for order of magnitude advances in our constraints on properties of dark energy and cosmology over the next decade.
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Juan Vidal O, Gandia C, Pardo-Sánchez J, Benet M, Aparisi S, Palanca S, Ansotegui E, Jordá C, Cerón J, Mancheño N, Sánchez-Céspedes M, Lahoz A, Carretero J, Farràs R. Development of primary human NSCLC patient derived xenograft and organoids models as a precision approach to tumor treatment. Ann Oncol 2018. [DOI: 10.1093/annonc/mdy303.052] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/13/2022] Open
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Ena J, Gómez-Huelgas R, Gracia-Tello B, Vázquez-Rodríguez P, Alcalá-Pedrajas J, Carrasco-Sánchez F, Murcia-Casas B, Romero-Sánchez M, Segura-Heras J, Carretero J. Derivation and validation of a predictive model for the readmission of patients with diabetes mellitus treated in internal medicine departments. Rev Clin Esp 2018. [DOI: 10.1016/j.rceng.2018.03.018] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/01/2022]
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Ena J, Gómez-Huelgas R, Gracia-Tello BC, Vázquez-Rodríguez P, Alcalá-Pedrajas JN, Carrasco-Sánchez FJ, Murcia-Casas B, Romero-Sánchez M, Segura-Heras JV, Carretero J. Derivation and validation of a predictive model for the readmission of patients with diabetes mellitus treated in internal medicine departments. Rev Clin Esp 2018; 218:271-278. [PMID: 29731294 DOI: 10.1016/j.rce.2018.03.010] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/11/2018] [Revised: 03/15/2018] [Accepted: 03/16/2018] [Indexed: 10/17/2022]
Abstract
OBJECTIVES We developed a predictive model for the hospital readmission of patients with diabetes. The objective was to identify the frail population that requires additional strategies to prevent readmissions at 90 days. METHODS Using data collected from 1977 patients in 3 studies on the national prevalence of diabetes (2015-2017), we developed and validated a predictive model of readmission at 90 days for patients with diabetes. RESULTS A total of 704 (36%) readmissions were recorded. There were no differences in the readmission rates over the course of the 3 studies. The hospitals with more than 500 beds showed significantly (p=.02) higher readmission rates than those with fewer beds. The main reasons for readmission were infectious diseases (29%), cardiovascular diseases (24) and respiratory diseases (14%). Readmissions directly related to diabetic decompensations accounted for only 2% of all readmissions. The independent variables associated with hospital readmission were patient's age, degree of comorbidity, estimated glomerular filtration rate, degree of disability, presence of previous episodes of hypoglycaemia, use of insulin in treating diabetes and the use of systemic glucocorticoids. The predictive model showed an area under the ROC curve (AUC) of 0.676 (95% confidence interval [95% CI] 0.642-0.709; p=.001) in the referral cohort. In the validation cohort, the model showed an AUC of 0.661 (95% CI 0.612-0.710; p=.001). CONCLUSION The model we developed for predicting readmissions for hospitalised patients with type 2 diabetes helps identify a subgroup of frail patients with a high risk of readmission.
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Guirado L, Crispi F, Masoller N, Bennasar M, Marimon E, Carretero J, Gratacós E, Martínez JM, Friedberg MK, Gómez O. Biventricular impact of mild to moderate fetal pulmonary valve stenosis. ULTRASOUND IN OBSTETRICS & GYNECOLOGY : THE OFFICIAL JOURNAL OF THE INTERNATIONAL SOCIETY OF ULTRASOUND IN OBSTETRICS AND GYNECOLOGY 2018; 51:349-356. [PMID: 28295792 DOI: 10.1002/uog.17456] [Citation(s) in RCA: 14] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/28/2016] [Revised: 02/02/2017] [Accepted: 02/28/2017] [Indexed: 06/06/2023]
Abstract
OBJECTIVES To define the pattern of fetal echocardiographic changes associated with isolated pulmonary valve stenosis (PS) and to correlate the echocardiographic findings with neonatal outcome and the need for postnatal pulmonary valvuloplasty within the first 12 months postpartum. METHODS This was a prospective cohort study between January 2009 and October 2015 of 16 fetuses with isolated PS and 48 controls matched by gestational age at ultrasound examination (± 2 weeks) evaluated at the Fetal Cardiology Unit at BCNatal (Barcelona). Standard fetal ultrasound and comprehensive echocardiography, which included cardiovascular morphometric parameters, and systolic and diastolic functional and timing measurements, were performed in all cases. Baseline characteristics and perinatal outcome were retrieved from clinical records. Cases were followed up until 12 months of age, and admission to intensive care unit, days of hospitalization, need for prostaglandins and requirement for postnatal surgery were reviewed. Fetal PS cases were analyzed according to the need for postnatal pulmonary valvuloplasty. RESULTS The study groups were similar in terms of baseline, fetal ultrasound and perinatal characteristics. Median gestational age at diagnosis of PS was 33.4 (range, 20.0-36.5) weeks. Most cases corresponded to mild or moderate PS; only three fetuses had reversed flow in the ductus arteriosus before delivery. Six (37.5%) newborns, including all three with reversed flow in the ductus arteriosus prenatally, required postnatal pulmonary valvuloplasty. Fetuses with PS presented with larger and more globular hearts, with increased myocardial wall thickness in the third trimester. Despite preserved right ventricular (RV) ejection fraction and systolic longitudinal motion, PS cases showed increased right cardiac output and signs of diastolic dysfunction, with higher ductus venosus pulsatility index (0.72 ± 0.32 vs 0.53 ± 0.16, P = 0.004) and tricuspid E/E' ratio (7.52 ± 3.07 vs 5.76 ± 1.79, P = 0.022). In addition, fetuses with PS displayed a compensatory increase in left ventricular (LV) radial and longitudinal motion, as shown by a higher ejection fraction (79.3 ± 8.23% vs 67.6 ± 11.3%, P = 0.003) and mitral annular-plane systolic excursion (5.94 ± 1.38 vs 5.0 ± 1.22 mm, P = 0.035). Finally, fetuses requiring postnatal pulmonary valvuloplasty showed a different pattern of echocardiographic findings from those not requiring valvuloplasty, with a significantly smaller RV and pulmonary valve diameter, reduced tricuspid annular-plane systolic excursion (5.08 ± 1.59 vs 8.07 ± 1.93 mm, P = 0.028), increased LV cardiac output (340 ± 16 vs 176 ± 44 mL/min/kg, P = 0.003) and more pronounced signs of LV diastolic dysfunction (mitral E' velocity, 5.78 ± 0.90 vs 8.16 ± 1.58 cm/s, P = 0.008). CONCLUSIONS Fetuses with PS present with more hypertrophic, larger and more globular hearts in the third trimester of pregnancy, associated with a higher right cardiac output and impaired biventricular relaxation. In addition, signs of increased LV contraction were observed. Our data suggest that RV and LV functional parameters could be useful for predicting the need for postnatal pulmonary valvuloplasty. Copyright © 2017 ISUOG. Published by John Wiley & Sons Ltd.
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Fernández L, Carretero J, Prada F, Caffarena J. Fístula aortocavitaria en endocarditis sobre válvula nativa. An Pediatr (Barc) 2015; 82:e266-7. [DOI: 10.1016/j.anpedi.2013.10.033] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/11/2013] [Revised: 10/05/2013] [Accepted: 10/17/2013] [Indexed: 11/16/2022] Open
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Soucheray M, Kikuchi E, Pulido I, Akbay E, Becker J, Christensen C, Johnson N, Patel T, Carretero J, Wong K, Shimamura T. 593 Strategies to overcome resistance to BET bromodomain inhibitor in KRAS/LKB1 mutant NSCLC. Eur J Cancer 2014. [DOI: 10.1016/s0959-8049(14)70719-1] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/28/2022]
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Pedescoll A, Sidrach-Cardona R, Sánchez JC, Carretero J, Garfi M, Bécares E. Design configurations affecting flow pattern and solids accumulation in horizontal free water and subsurface flow constructed wetlands. WATER RESEARCH 2013; 47:1448-1458. [PMID: 23286990 DOI: 10.1016/j.watres.2012.12.010] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/20/2012] [Revised: 12/05/2012] [Accepted: 12/07/2012] [Indexed: 06/01/2023]
Abstract
The aim of this study was to evaluate the effect of different horizontal constructed wetland (CW) design parameters on solids distribution, loss of hydraulic conductivity over time and hydraulic behaviour, in order to assess clogging processes in wetlands. For this purpose, an experimental plant with eight CWs was built at mesocosm scale. Each CW presented a different design characteristic, and the most common CW configurations were all represented: free water surface flow (FWS) with different effluent pipe locations, FWS with floating macrophytes and subsurface flow (SSF), and the presence of plants and specific species (Typha angustifolia and Phragmites australis) was also considered. The loss of the hydraulic conductivity of gravel was greatly influenced by the presence of plants and organic load (representing a loss of 20% and c.a. 10% in planted wetlands and an overloaded system, respectively). Cattail seems to have a greater effect on the development of clogging since its below-ground biomass weighed twice as much as that of common reed. Hydraulic behaviour was greatly influenced by the presence of a gravel matrix and the outlet pipe position. In strict SSF CW, the water was forced to cross the gravel and tended to flow diagonally from the top inlet to the bottom outlet (where the inlet and outlet pipes were located). However, when FWS was considered, water preferentially flowed above the gravel, thus losing half the effective volume of the system. Only the presence of plants seemed to help the water flow partially within the gravel matrix.
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Vazquez T, Sañudo JR, Carretero J, Parkin I, Rodríguez-Niedenführ M. Variations of the radial recurrent artery of clinical interest. Surg Radiol Anat 2013; 35:689-94. [PMID: 23440497 DOI: 10.1007/s00276-013-1094-4] [Citation(s) in RCA: 9] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/26/2012] [Accepted: 02/16/2013] [Indexed: 10/27/2022]
Abstract
PURPOSE The anatomy of the radial recurrent artery (RRA) is important for different clinical procedures: interventional cardiology and microsurgery of the forearm; however, few studies have analysed its morphology: number, course, relations and distribution. METHODS The RRA was analysed in 332 upper limbs divided into two groups: (1) normal pattern of the arterial axis of the upper limb (266 cases), (2) associated with major arterial variations (66 cases). RESULTS A second or accessory RRA existed in 31.2 % in group 1, and 30.3 % in group 2. In both groups, the second RRA originated from the brachial (100 %) and always (100 %) coursed behind the bicipital tendon. The accessory RRA supplied the brachioradialis, brachialis and biceps brachii muscles. The RRA in group 1, originated mostly from the radial artery (75 %), followed by radioulnar division and ulno-interosseous trunk. In group 2, the RRA arise from the brachioradial artery (65 %), or from the radial artery (in cases of ulnar or brachial artery variation). The course of the RRA behind the biceps brachii tendon was observed in 9.4 % of group 1 and in 6.1 % of group 2. The RRA supplied the brachioradialis, extensor carpi radialis longus and brevis, and supinator muscles. The RRA and accessory RRA anastomosed forming a ring around the biceps brachii tendon in 0.75 % in group 1 and in 13.6 % in group 2, the latter group having an important clinical interest. CONCLUSIONS The variability of the RRA may provide an advantage for microsurgical procedures of the elbow and disadvantage during transradial catheterism.
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