Observation of Gravitational Waves from a Binary Black Hole Merger

On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0×10(-21). It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203,000 years, equivalent to a significance greater than 5.1σ. The source lies at a luminosity distance of 410(-180)(+160)  Mpc corresponding to a redshift z=0.09(-0.04)(+0.03). In the source frame, the initial black hole masses are 36(-4)(+5)M⊙ and 29(-4)(+4)M⊙, and the final black hole mass is 62(-4)(+4)M⊙, with 3.0(-0.5)(+0.5)M⊙c(2) radiated in gravitational waves. All uncertainties define 90% credible intervals. These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.

Cloning of senescent cell-derived inhibitors of DNA synthesis using an expression screen

We here describe a rapid and simple expression screen method that has allowed us to isolate cDNAs coding for inhibitors of DNA synthesis from senescent human diploid fibroblasts. The assay involved transient transcriptional overexpression of a gene product encoded by a cDNA in a proliferating cell, on the assumption that this would be sufficient to block DNA synthesis in a short-term assay using tritiated thymidine autoradiography. Three cDNAs, referred to as senescent cell-derived inhibitors (sdi), that exhibit DNA synthesis-inhibitory activity when introduced into young cycling cells, were successfully identified. Expression of one of the cDNAs, sdi1, increased 10- to 20-fold in senescent compared with young cells and the increase in RNA closely paralleled the onset of the senescent phenotype and loss of cell proliferation. sdi1 expression was also increased in young cells made nondividing (quiescent) by deprivation of growth factors or contact inhibition. Following serum stimulation, RNA levels of sdi1 in quiescent cells were initially increased, but then declined to low levels just prior to the entry of the cells into S phase. In contrast, RNA levels of sdi1 in senescent cells failed to decline, suggesting a role for this gene in maintaining the senescent phenotype. The sdi1 gene has been mapped to the p arm of chromosome 6.

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

On August 17, 2017 at 12∶41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×10^{4}  years. We infer the component masses of the binary to be between 0.86 and 2.26  M_{⊙}, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60  M_{⊙}, with the total mass of the system 2.74_{-0.01}^{+0.04}M_{⊙}. The source was localized within a sky region of 28  deg^{2} (90% probability) and had a luminosity distance of 40_{-14}^{+8}  Mpc, the closest and most precisely localized gravitational-wave signal yet. The association with the γ-ray burst GRB 170817A, detected by Fermi-GBM 1.7 s after the coalescence, corroborates the hypothesis of a neutron star merger and provides the first direct evidence of a link between these mergers and short γ-ray bursts. Subsequent identification of transient counterparts across the electromagnetic spectrum in the same location further supports the interpretation of this event as a neutron star merger. This unprecedented joint gravitational and electromagnetic observation provides insight into astrophysics, dense matter, gravitation, and cosmology.

Modulation of non-templated nucleotide addition by Taq DNA polymerase: primer modifications that facilitate genotyping

Taq DNA polymerase can catalyze non-templated addition of a nucleotide (principally adenosine) to the 3' end of PCR-amplified products. Recently, we showed that this activity, which is primer-specific, presents a potential source of error in genotyping studies based on the use of short tandem repeat (STR) markers. Furthermore, in reviewing our data, we found that non-templated nucleotide addition adjacent to a 3' terminal C is favored and that addition adjacent to a 3' terminal A is not. It was clear, however, that features of the template in addition to the 3' terminal base also affect the fraction of product adenylated. To define consensus sequences that promote or inhibit product adenylation, we transplanted sequences between the 5' ends of the reverse primers of markers that are adenylated and those of markers that are not adenylated. It proved difficult to identify a single sequence capable of protecting the products of all markers from non-templated addition of nucleotide. On the other hand, placing the sequence GTTTCTT on the 5' end of reverse primers resulted in nearly 100% adenylation of the 3' end of the forward strand. This modification or related ones (called "PIG-tailing") should facilitate accurate genotyping and efficient T/A cloning.

Major susceptibility locus for prostate cancer on chromosome 1 suggested by a genome-wide search

Despite its high prevalence, very little is known regarding genetic predisposition to prostate cancer. A genome-wide scan performed in 66 high-risk prostate cancer families has provided evidence of linkage to the long arm of chromosome 1 (1q24-25). Analysis of an additional set of 25 North American and Swedish families with markers in this region resulted in significant evidence of linkage in the combined set of 91 families. The data provide strong evidence of a major prostate cancer susceptibility locus on chromosome 1.

Prevalence of nonconvulsive status epilepticus in comatose patients

BACKGROUND

Nonconvulsive status epilepticus (NCSE) is a form of status epilepticus (SE) that is an often unrecognized cause of coma.

OBJECTIVE

To evaluate the presence of NCSE in comatose patients with no clinical signs of seizure activity.

METHODS

A total of 236 patients with coma and no overt clinical seizure activity were monitored with EEG as part of their coma evaluation. This study was conducted during our prospective evaluation of SE, where it has been validated that we identify over 95% of all SE cases at the Medical College of Virginia Hospitals. Only cases that were found to have no clinical signs of SE were included in this study.

RESULTS

EEG demonstrated that 8% of these patients met the criteria for the diagnosis of NCSE. The study included an age range from 1 month to 87 years.

CONCLUSION

This large-scale EEG evaluation of comatose patients without clinical signs of seizure activity found that NCSE is an underrecognized cause of coma, occurring in 8% of all comatose patients without signs of seizure activity. EEG should be included in the routine evaluation of comatose patients even if clinical seizure activity is not apparent.

Replicative senescence: implications for in vivo aging and tumor suppression

Normal cells have limited proliferative potential in culture, a fact that has been the basis of their use as a model for replicative senescence for many years. Recent molecular analyses have identified numerous changes in gene expression that occur as cells become senescent, and the results indicate that multiple levels of control contribute to the irreversible growth arrest. These include repression of growth stimulatory genes, overexpression of growth inhibitory genes, and interference with downstream pathways. Studies with cell types other than fibroblasts will better define the role of cell senescence in the aging process and in tumorigenesis.

CCAAT/enhancer-binding protein alpha (C/EBP alpha) inhibits cell proliferation through the p21 (WAF-1/CIP-1/SDI-1) protein

C/EBPalpha has a role in growth arrest and differentiation of mouse preadipocytes. To study the mechanism of C/EBPalpha-induced growth arrest, we developed a cell line, HT1, that contained the human C/EBPalpha gene under Lac repressor control. IPTG-induced C/EBPalpha caused inhibition of cell proliferation and DNA synthesis as measured by colony growth assays, cell counting, and BrdU uptake. A number of proteins that are known to be involved in the regulation of the cell cycle, such as cyclin-dependent kinase (CDK)2 and CDK4, proliferating cell nuclear antigen (PCNA), p53, c-fos, and the CDK inhibitor p16 and p27 were investigated by Western analysis. No change in their expression was observed. However, the p21 (WAF-1/CIP-1/SDI-1) protein was significantly elevated in growth-arrested HT1 cells. Elevation of p21/SDI-1 mRNA (threefold) and activation of the p21/SDI-1 promoter by C/EBPalpha did not account for the 12- to 20-fold increase in p21/SDI-1 protein. Protein synthesis inhibition by cycloheximide (CHX) treatment indicated that the half-life of p21/SDI-1 in dividing HT1 cells was approximately 30 min. However, in C/EBPalpha growth-arrested cells, the level of the p21/SDI-1 did not change for > 80 min after CHX addition. Our studies demonstrate that C/EBPalpha activates p21/SDI-1 by increasing p21/SDI-1 gene expression and by post-translational stabilization of p21/SDI-1 protein. Furthermore, induction of p21/SDI-1 is responsible for the ability of C/EBPalpha to inhibit proliferation because transcription of antisense p21/SDI-1 mRNA eliminated growth inhibition by C/EBPalpha.

GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

We report the observation of a gravitational-wave signal produced by the coalescence of two stellar-mass black holes. The signal, GW151226, was observed by the twin detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) on December 26, 2015 at 03:38:53 UTC. The signal was initially identified within 70 s by an online matched-filter search targeting binary coalescences. Subsequent off-line analyses recovered GW151226 with a network signal-to-noise ratio of 13 and a significance greater than 5σ. The signal persisted in the LIGO frequency band for approximately 1 s, increasing in frequency and amplitude over about 55 cycles from 35 to 450 Hz, and reached a peak gravitational strain of 3.4_{-0.9}^{+0.7}×10^{-22}. The inferred source-frame initial black hole masses are 14.2_{-3.7}^{+8.3}M_{⊙} and 7.5_{-2.3}^{+2.3}M_{⊙}, and the final black hole mass is 20.8_{-1.7}^{+6.1}M_{⊙}. We find that at least one of the component black holes has spin greater than 0.2. This source is located at a luminosity distance of 440_{-190}^{+180}  Mpc corresponding to a redshift of 0.09_{-0.04}^{+0.03}. All uncertainties define a 90% credible interval. This second gravitational-wave observation provides improved constraints on stellar populations and on deviations from general relativity.

Genetic analysis of indefinite division in human cells: identification of four complementation groups

Hybrids obtained following fusion of normal human diploid fibroblasts with different immortal human cell lines exhibited limited division potential. This led to the conclusion that the phenotype of cellular senescence is dominant and that immortal cells arise as a result of recessive changes in the growth control mechanisms of the normal cell. We have exploited the fact that immortality is recessive and, by fusing immortal human cell lines with each other, assigned 21 cell lines to at least four complementation groups for indefinite division. A wide variety of cell lines was included in the study to determine what parameters, if any, would affect complementation group assignment. The results indicate that cell type, embryonal layer of origin, and type of tumor do not affect group assignment. There does not appear to be any correlation between expression of an activated oncogene and group assignment. However, all of the immortal simian virus 40-transformed cell lines studied (with the exception of one xerodermapigmentosum fibroblast-derived line) assign to the same group, indicating that this virus immortalizes various human cells by the same processes. The assignment of immortal human cells to distinct groups provides the basis for a focused approach to determine the genes important in normal growth regulation that have been modified in immortal cells.

Differential efficacy of tumor necrosis factor inhibition in the management of inflammatory eye disease and associated rheumatic disease

OBJECTIVE

To evaluate the clinical usefulness of tumor necrosis factor (TNF) inhibitors in patients with inflammatory eye disease that is resistant to conventional immunosuppressive therapies.

METHODS

Sixteen patients (4 males and 12 females aged 7 to 78 years) who received etanercept (n = 14) or infliximab (n = 2) for either inflammatory eye disease or associated joint disease were studied retrospectively to determine the effect of these medications on their ocular inflammation.

RESULTS

Nine cases of uveitis and 7 cases of scleritis were treated. Systemic diagnoses included rheumatoid arthritis (n = 8), juvenile rheumatoid arthritis (n = 3), ankylosing spondylitis (n = 1), and psoriatic spondylarthropathy (n = 1). Three patients had uveitis without associated systemic disease. Although 12 of 12 patients with active articular inflammation (100%) experienced improvement in joint disease, only 6 of 16 with ocular inflammation (38%) experienced improvement in eye disease. Five patients developed inflammatory eye disease for the first time while taking a TNF inhibitor. No patient discontinued treatment because of adverse drug effects.

CONCLUSION

TNF inhibitors are well tolerated immunosuppressive medications that may benefit certain subgroups of patients with inflammatory eye disease, but they appear to be more effective in controlling associated inflammatory arthritis.

Variation in the life-span of clones derived from human diploid cell strains

The doubling potential of several hundred clones derived from WI-38 and WI-26 cell cultures has been determined. Clones were isolated at various population doubling levels (PDLs) during the finite in vitro life-span of the mass (uncloned) cultures. In all cases, there was a large variation in population doubling potential (or life-span) among the clones isolated from a single mass culture. When clones were isolated from mass cultures which had undergone eight or nine population doublings, only about 50% of the clones were capable of more than eight population doublings. This percentage was further reduced when clones were isolated from mass cultures at higher PDLs. Mass cultures appear to be composed of two subpopulation classes: one with a low population doubling potential, and the other with a higher population doubling potential. Nevertheless, the highest doubling potential observed in clones isolated from any single culture was about the same as the doubling potential of the mass culture from which single cells were taken.

Evidence for the recessive nature of cellular immortality

Fusion of immortal cell lines with normal human fibroblasts or certain other immortal cell lines yields hybrids having limited division potential. Cellular immortality was found to be a recessive phenotype in hybrids. It was also found that at least two separate events in the normal cell genome can result in immortality. In fusions involving certain immortal parent cells, these events can be complemented to result in hybrids with finite division capacity.

Intraclonal variation in proliferative potential of human diploid fibroblasts: stochastic mechanism for cellular aging

At several points during the growth of a clone of human embryonic lung fibroblasts in vitro, 100 to 200 cells were removed at random and the proliferative potential of each cell was determined. At each sample point, a wide variation in remaining population doubling ability was observed among the individual cells and the distributions of doubling potentials were distinctly bimodal. Furthermore, the two cells arising from a single mitosis differed in their ability to proliferate by as many as eight population doublings (256-fold in the number of cells produced). The results suggest that a stochastic process is responsible for determining the limited proliferative potential of human embryonic lung fibroblasts.

GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

We describe the observation of GW170104, a gravitational-wave signal produced by the coalescence of a pair of stellar-mass black holes. The signal was measured on January 4, 2017 at 10∶11:58.6 UTC by the twin advanced detectors of the Laser Interferometer Gravitational-Wave Observatory during their second observing run, with a network signal-to-noise ratio of 13 and a false alarm rate less than 1 in 70 000 years. The inferred component black hole masses are 31.2_{-6.0}^{+8.4}M_{⊙} and 19.4_{-5.9}^{+5.3}M_{⊙} (at the 90% credible level). The black hole spins are best constrained through measurement of the effective inspiral spin parameter, a mass-weighted combination of the spin components perpendicular to the orbital plane, χ_{eff}=-0.12_{-0.30}^{+0.21}. This result implies that spin configurations with both component spins positively aligned with the orbital angular momentum are disfavored. The source luminosity distance is 880_{-390}^{+450}  Mpc corresponding to a redshift of z=0.18_{-0.07}^{+0.08}. We constrain the magnitude of modifications to the gravitational-wave dispersion relation and perform null tests of general relativity. Assuming that gravitons are dispersed in vacuum like massive particles, we bound the graviton mass to m_{g}≤7.7×10^{-23}  eV/c^{2}. In all cases, we find that GW170104 is consistent with general relativity.

GW170817: Measurements of Neutron Star Radii and Equation of State

On 17 August 2017, the LIGO and Virgo observatories made the first direct detection of gravitational waves from the coalescence of a neutron star binary system. The detection of this gravitational-wave signal, GW170817, offers a novel opportunity to directly probe the properties of matter at the extreme conditions found in the interior of these stars. The initial, minimal-assumption analysis of the LIGO and Virgo data placed constraints on the tidal effects of the coalescing bodies, which were then translated to constraints on neutron star radii. Here, we expand upon previous analyses by working under the hypothesis that both bodies were neutron stars that are described by the same equation of state and have spins within the range observed in Galactic binary neutron stars. Our analysis employs two methods: the use of equation-of-state-insensitive relations between various macroscopic properties of the neutron stars and the use of an efficient parametrization of the defining function p(ρ) of the equation of state itself. From the LIGO and Virgo data alone and the first method, we measure the two neutron star radii as R_{1}=10.8_{-1.7}^{+2.0}  km for the heavier star and R_{2}=10.7_{-1.5}^{+2.1}  km for the lighter star at the 90% credible level. If we additionally require that the equation of state supports neutron stars with masses larger than 1.97  M_{⊙} as required from electromagnetic observations and employ the equation-of-state parametrization, we further constrain R_{1}=11.9_{-1.4}^{+1.4}  km and R_{2}=11.9_{-1.4}^{+1.4}  km at the 90% credible level. Finally, we obtain constraints on p(ρ) at supranuclear densities, with pressure at twice nuclear saturation density measured at 3.5_{-1.7}^{+2.7}×10^{34}  dyn cm^{-2} at the 90% level.

Replicative senescence of human skin fibroblasts correlates with a loss of regulation and overexpression of collagenase activity

The atrophy of extracellular matrix is a common event during the aging of connective tissues. In this study, we tested the hypothesis that the altered ability of senescent cells to be modulated by serum growth factors correlated with a loss of regulation of collagenase synthesis. We examined the levels of immunoreactive procollagenase and collagenase inhibitor (the tissue inhibitor of metalloproteinases, TIMP) associated with young and senescent fibroblasts cultured in vitro. Young fibroblasts cultured in low (0.5%) concentrations of fetal bovine serum respond to increased (10%) serum by increasing levels of procollagenase and TIMP beginning 4.0 h after serum stimulation. In contrast, senescent fibroblasts constitutively produce relatively high levels of procollagenase even when cultured in low levels of serum and do not respond to serum stimulation by increasing procollagenase synthesis. In addition, senescent fibroblasts constitutively express a relatively small amount of TIMP which is not induced upon serum stimulation. This altered expression of collagenase and TIMP appears unique to the senescent phenotype and not merely a result of growth inhibition, since young cells growth arrested by density-dependent growth inhibition displayed a temporal pattern of procollagenase and TIMP expression upon serum stimulation similar to that of subconfluent young cultures. An assay of net collagenase activity revealed a greater than 20-fold elevation of activity in trypsin-activated extracts from senescent versus young fibroblasts when cultured in a low concentration of fetal bovine serum. These results demonstrate for the first time a direct correlation between alterations in the molecular pathways regulating connective tissue homeostasis and those of replicative senescence. The increased collagenolytic activity of senescent compared to young fibroblasts cultured in the presence of a low serum concentration suggests that aging fibroblasts may become increasingly fibroclastic causing many of the age-associated alterations in dermal collagen observed during aging in vivo.

Smokers' polycythemia

Twenty-two smokers with elevated hematocrits (mean, 54 per cent) had elevated blood carboxyhemoglobin (mean, 11.6 per cent; normal, less than 1 per cent) and a "left-shifted" oxygen-hemoglobin dissociation curve (mean P50, 21.6 +/- 2.3 [+/- S.D.] torr; normal, 26.7 +/- 1.1). Red-cell volume was increased in 14 of 18, and plasma volume reduced in 14 of 18. Fatigue and headache were common, and syncopal attacks occurred in four patients. Symptoms disappeared and the elevated red-cell volume decreased markedly in all five patients who were able to reduce severely their smoking habit; low plasma volume increased in three of four patients studied. We conclude that carbon monoxide exposure from cigar and cigarette smoke is a frequent cause of an elevated red-cell volume or a reduced plasma volume (or both). Measurement of carboxyhemoglobin should be a routine part of the evaluation of all polycythemic subjects.

Tests of General Relativity with GW150914

The LIGO detection of GW150914 provides an unprecedented opportunity to study the two-body motion of a compact-object binary in the large-velocity, highly nonlinear regime, and to witness the final merger of the binary and the excitation of uniquely relativistic modes of the gravitational field. We carry out several investigations to determine whether GW150914 is consistent with a binary black-hole merger in general relativity. We find that the final remnant's mass and spin, as determined from the low-frequency (inspiral) and high-frequency (postinspiral) phases of the signal, are mutually consistent with the binary black-hole solution in general relativity. Furthermore, the data following the peak of GW150914 are consistent with the least-damped quasinormal mode inferred from the mass and spin of the remnant black hole. By using waveform models that allow for parametrized general-relativity violations during the inspiral and merger phases, we perform quantitative tests on the gravitational-wave phase in the dynamical regime and we determine the first empirical bounds on several high-order post-Newtonian coefficients. We constrain the graviton Compton wavelength, assuming that gravitons are dispersed in vacuum in the same way as particles with mass, obtaining a 90%-confidence lower bound of 10^{13}  km. In conclusion, within our statistical uncertainties, we find no evidence for violations of general relativity in the genuinely strong-field regime of gravity.

Nitric oxide production by human intestinal epithelial cells and competition for arginine as potential determinants of host defense against the lumen-dwelling pathogen Giardia lamblia

Giardia lamblia infection of the human small intestine is a common protozoan cause of diarrheal disease worldwide. Although infection is luminal and generally self-limiting, and secretory Abs are thought to be important in host defense, other defense mechanisms probably affect the duration of infection and the severity of symptoms. Because intestinal epithelial cells produce NO, and its stable end products, nitrite and nitrate, are detectable mainly on the apical side, we tested the hypothesis that NO production may constitute a host defense against G. lamblia. Several NO donors, but not their control compounds, inhibited giardial growth without affecting viability, suggesting that NO is cytostatic rather than cytotoxic for G. lamblia. NO donors also inhibited giardial differentiation induced by modeling crucial environmental factors, i. e., encystation induced by bile and alkaline pH, and excystation in response to gastric pH followed by alkaline pH and protease. Despite the potent antigiardial activity of NO, G. lamblia is not simply a passive target for host-produced NO, but has strategies to evade this potential host defense. Thus, in models of human intestinal epithelium, G. lamblia inhibited epithelial NO production by consuming arginine, the crucial substrate used by epithelial NO synthase to form NO. These studies define NO and arginine as central components in a novel cross-talk between a luminal pathogen and host intestinal epithelium.

Safety study of nonoxynol-9 as a vaginal microbicide: evidence of adverse effects

Nonoxynol-9 (N-9) is virucidal in vitro, and is therefore a candidate microbicide for preventing sexual transmission of HIV. However, the activity of N-9 is nonspecific, suggesting that virucidal levels may produce adverse effects including epithelial disruption, inflammation of the genital mucosa, or both. A randomized placebo controlled trial of daily use of 100 mg of N-9 took place for 1 week in 40 female volunteers. Outcome measures included symptoms, colposcopic and histologic changes in the genital tract, and impact on vaginal flora. Genital irritation was reported by 10 of the N-9 and 5 of the placebo group. Colposcopy showed erythema in 9 of the N-9 group and 2 of the placebo group. Histologic inflammation was found in 7 of the N-9 group and 2 of the placebo group. Inflammatory changes were characterized by patchy infiltration of the lamina propria predominantly with CD8+ lymphocytes and macrophages, in the absence of epithelial disruption. A transient reduction in numbers of lactobacilli was observed in 9 of the 15 women using N-9, and 6 of 18 women using placebo. N-9 used for 7 days in a standard spermicidal dose was associated with increased irritation, colposcopic and histologic evidence of inflammation and was more frequently associated with reduction in numbers of lactobacilli during gel use. The clinical significance of the recruitment of cells susceptible to HIV infection to the genital mucosa is unknown but raises concerns about the suitability of N-9 as a microbicide when given in this dose.

Existence of high abundance antiproliferative mRNA's in senescent human diploid fibroblasts

Polyadenylated RNA isolated from senescent human diploid fibroblasts (HDF) inhibited DNA synthesis in proliferation-competent cells after microinjection, whereas polyadenylated RNA from young HDF had no inhibitory effect. Polyadenylated RNA from young cells made quiescent by removal of serum growth factors had a slight inhibitory effect on DNA synthesis. The abundance level of inhibitor messenger RNA (mRNA) from senescent cells was estimated at 0.8 and that of quiescent cells at 0.005 percent. These results demonstrate the existence of one or more antiproliferative mRNA's in nonproliferating normal human cells; these RNA's code for factors that either work antagonistically to initiators of DNA synthesis or regulate the expression of the initiators in some way. The abundance level of the inhibitory mRNA in senescent cells indicates the feasibility of developing a complementary DNA probe that will be useful in studying cell cycle control mechanisms.