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Showing papers by "University of Leicester published in 2017"


Journal ArticleDOI
TL;DR: The Global Burden of Diseases, Injuries, and Risk Factors Study 2016 (GBD 2016) provides a comprehensive assessment of prevalence, incidence, and years lived with disability (YLDs) for 328 causes in 195 countries and territories from 1990 to 2016.

10,401 citations


Journal ArticleDOI
TL;DR: Intratumor heterogeneity mediated through chromosome instability was associated with an increased risk of recurrence or death, a finding that supports the potential value of chromosome instability as a prognostic predictor.
Abstract: BackgroundAmong patients with non–small-cell lung cancer (NSCLC), data on intratumor heterogeneity and cancer genome evolution have been limited to small retrospective cohorts. We wanted to prospectively investigate intratumor heterogeneity in relation to clinical outcome and to determine the clonal nature of driver events and evolutionary processes in early-stage NSCLC. MethodsIn this prospective cohort study, we performed multiregion whole-exome sequencing on 100 early-stage NSCLC tumors that had been resected before systemic therapy. We sequenced and analyzed 327 tumor regions to define evolutionary histories, obtain a census of clonal and subclonal events, and assess the relationship between intratumor heterogeneity and recurrence-free survival. ResultsWe observed widespread intratumor heterogeneity for both somatic copy-number alterations and mutations. Driver mutations in EGFR, MET, BRAF, and TP53 were almost always clonal. However, heterogeneous driver alterations that occurred later in evolution w...

1,679 citations


Journal ArticleDOI
23 Feb 2017-Nature
TL;DR: The observations reveal that at least seven planets with sizes and masses similar to those of Earth revolve around TRAPPIST-1, and the six inner planets form a near-resonant chain, such that their orbital periods are near-ratios of small integers.
Abstract: One aim of modern astronomy is to detect temperate, Earth-like exoplanets that are well suited for atmospheric characterization. Recently, three Earth-sized planets were detected that transit (that is, pass in front of) a star with a mass just eight per cent that of the Sun, located 12 parsecs away. The transiting configuration of these planets, combined with the Jupiter-like size of their host star—named TRAPPIST-1—makes possible in-depth studies of their atmospheric properties with present-day and future astronomical facilities. Here we report the results of a photometric monitoring campaign of that star from the ground and space. Our observations reveal that at least seven planets with sizes and masses similar to those of Earth revolve around TRAPPIST-1. The six inner planets form a near-resonant chain, such that their orbital periods (1.51, 2.42, 4.04, 6.06, 9.1 and 12.35 days) are near-ratios of small integers. This architecture suggests that the planets formed farther from the star and migrated inwards. Moreover, the seven planets have equilibrium temperatures low enough to make possible the presence of liquid water on their surfaces.

1,476 citations


Journal ArticleDOI
08 Nov 2017-Nature
TL;DR: The fully integrated functionality and small size of Neuropixels probes allowed large populations of neurons from several brain structures to be recorded in freely moving animals and opens a path towards recording of brain-wide neural activity during behaviour.
Abstract: New silicon probes known as Neuropixels are shown to record from hundreds of neurons simultaneously in awake and freely moving rodents. Sensory, motor and cognitive operations involve the coordinated action of large neuronal populations across multiple brain regions. Existing technologies reliably measure activity from a relatively small number of neurons with high spatial and temporal resolution, or from a large volume of neurons with low resolution. Timothy Harris and colleagues describe the design, fabrication and performance of Neuropixels, a silicon probe that can measure well-isolated neural activity from hundreds of neurons. They integrated these probes into a lightweight system that could record activity simultaneously and with high fidelity from hundreds of neurons in awake and freely moving rodents. Sensory, motor and cognitive operations involve the coordinated action of large neuronal populations across multiple brain regions in both superficial and deep structures1,2. Existing extracellular probes record neural activity with excellent spatial and temporal (sub-millisecond) resolution, but from only a few dozen neurons per shank. Optical Ca2+ imaging3,4,5 offers more coverage but lacks the temporal resolution needed to distinguish individual spikes reliably and does not measure local field potentials. Until now, no technology compatible with use in unrestrained animals has combined high spatiotemporal resolution with large volume coverage. Here we design, fabricate and test a new silicon probe known as Neuropixels to meet this need. Each probe has 384 recording channels that can programmably address 960 complementary metal–oxide–semiconductor (CMOS) processing-compatible low-impedance TiN6 sites that tile a single 10-mm long, 70 × 20-μm cross-section shank. The 6 × 9-mm probe base is fabricated with the shank on a single chip. Voltage signals are filtered, amplified, multiplexed and digitized on the base, allowing the direct transmission of noise-free digital data from the probe. The combination of dense recording sites and high channel count yielded well-isolated spiking activity from hundreds of neurons per probe implanted in mice and rats. Using two probes, more than 700 well-isolated single neurons were recorded simultaneously from five brain structures in an awake mouse. The fully integrated functionality and small size of Neuropixels probes allowed large populations of neurons from several brain structures to be recorded in freely moving animals. This combination of high-performance electrode technology and scalable chip fabrication methods opens a path towards recording of brain-wide neural activity during behaviour.

1,443 citations


Journal ArticleDOI
Christopher Abbosh1, Nicolai Juul Birkbak1, Nicolai Juul Birkbak2, Gareth A. Wilson1, Gareth A. Wilson2, Mariam Jamal-Hanjani1, Tudor Constantin3, Raheleh Salari3, John Le Quesne4, David A. Moore4, Selvaraju Veeriah1, Rachel Rosenthal1, Teresa Marafioti1, Eser Kirkizlar3, Thomas B.K. Watkins2, Thomas B.K. Watkins1, Nicholas McGranahan2, Nicholas McGranahan1, Sophia Ward1, Sophia Ward2, Luke Martinson4, Joan Riley4, Francesco Fraioli1, Maise Al Bakir2, Eva Grönroos2, Francisco Zambrana1, Raymondo Endozo1, Wenya Linda Bi5, Wenya Linda Bi6, Fiona M. Fennessy5, Fiona M. Fennessy6, Nicole Sponer3, Diana Johnson1, Joanne Laycock1, Seema Shafi1, Justyna Czyzewska-Khan1, Andrew Rowan2, Tim Chambers2, Nik Matthews7, Nik Matthews2, Samra Turajlic2, Samra Turajlic8, Crispin T. Hiley2, Crispin T. Hiley1, Siow Ming Lee1, Martin Forster1, Tanya Ahmad1, Mary Falzon1, Elaine Borg1, David Lawrence1, Martin Hayward1, Shyam Kolvekar1, Nikolaos Panagiotopoulos1, Sam M. Janes1, Ricky Thakrar1, Asia Ahmed1, Fiona H Blackhall9, Yvonne Summers, Dina Hafez3, Ashwini Naik3, Apratim Ganguly3, Stephanie Kareht3, Rajesh Shah, Leena Dennis Joseph, Anne Marie Quinn, Phil Crosbie, Babu Naidu10, Gary Middleton10, Gerald Langman, Simon Trotter, Marianne Nicolson11, Hardy Remmen11, Keith M. Kerr11, Mahendran Chetty11, Lesley Gomersall11, Dean A. Fennell4, Apostolos Nakas12, Sridhar Rathinam12, Girija Anand13, Sajid Khan14, Peter Russell15, Veni Ezhil16, Babikir Ismail17, Melanie Irvin-Sellers17, Vineet Prakash17, Jason F. Lester18, Malgorzata Kornaszewska19, Richard Attanoos19, Haydn Adams18, Helen E. Davies18, Dahmane Oukrif1, Ayse U. Akarca1, John A. Hartley1, Helen Lowe1, Sara Lock20, Natasha Iles1, Harriet Bell1, Yenting Ngai1, Greg Elgar2, Zoltan Szallasi21, Zoltan Szallasi22, Zoltan Szallasi23, Roland F. Schwarz24, Javier Herrero1, Aengus Stewart2, Sergio A. Quezada1, Karl S. Peggs1, Peter Van Loo25, Peter Van Loo2, Caroline Dive1, Caroline Dive9, C. Jimmy Lin3, Matthew Rabinowitz3, Hugo J.W.L. Aerts5, Hugo J.W.L. Aerts6, Allan Hackshaw1, Jacqui Shaw4, Bernhard Zimmermann3, Charles Swanton1, Charles Swanton2 
25 May 2017-Nature
TL;DR: It is shown that phylogenetic ct DNA profiling tracks the subclonal nature of lung cancer relapse and metastasis, providing a new approach for ctDNA-driven therapeutic studies.
Abstract: The early detection of relapse following primary surgery for non-small-cell lung cancer and the characterization of emerging subclones, which seed metastatic sites, might offer new therapeutic approaches for limiting tumour recurrence. The ability to track the evolutionary dynamics of early-stage lung cancer non-invasively in circulating tumour DNA (ctDNA) has not yet been demonstrated. Here we use a tumour-specific phylogenetic approach to profile the ctDNA of the first 100 TRACERx (Tracking Non-Small-Cell Lung Cancer Evolution Through Therapy (Rx)) study participants, including one patient who was also recruited to the PEACE (Posthumous Evaluation of Advanced Cancer Environment) post-mortem study. We identify independent predictors of ctDNA release and analyse the tumour-volume detection limit. Through blinded profiling of postoperative plasma, we observe evidence of adjuvant chemotherapy resistance and identify patients who are very likely to experience recurrence of their lung cancer. Finally, we show that phylogenetic ctDNA profiling tracks the subclonal nature of lung cancer relapse and metastasis, providing a new approach for ctDNA-driven therapeutic studies.

1,179 citations


Journal ArticleDOI
TL;DR: The proposed LD Hub database and accompanying web interface will ensure maximal uptake of the LD score regression methodology, provide a useful database for the public dissemination of GWAS results, and provide a method for easily screening hundreds of traits for overlapping genetic aetiologies.
Abstract: Motivation: LD score regression is a reliable and efficient method of using genome-wide association study (GWAS) summary-level results data to estimate the SNP heritability of complex traits and diseases, partition this heritability into functional categories, and estimate the genetic correlation between different phenotypes. Because the method relies on summary level results data, LD score regression is computationally tractable even for very large sample sizes. However, publicly available GWAS summary-level data are typically stored in different databases and have different formats, making it difficult to apply LD score regression to estimate genetic correlations across many different traits simultaneously. Results: In this manuscript, we describe LD Hub - a centralized database of summary-level GWAS results for 173 diseases/traits from different publicly available resources/consortia and a web interface that automates the LD score regression analysis pipeline. To demonstrate functionality and validate our software, we replicated previously reported LD score regression analyses of 49 traits/diseases using LD Hub; and estimated SNP heritability and the genetic correlation across the different phenotypes. We also present new results obtained by uploading a recent atopic dermatitis GWAS meta-analysis to examine the genetic correlation between the condition and other potentially related traits. In response to the growing availability of publicly accessible GWAS summary-level results data, our database and the accompanying web interface will ensure maximal uptake of the LD score regression methodology, provide a useful database for the public dissemination of GWAS results, and provide a method for easily screening hundreds of traits for overlapping genetic aetiologies

854 citations


Journal ArticleDOI
16 Oct 2017-Nature
TL;DR: The spectral identification and physical properties of a bright kilonova associated with the gravitational-wave source GW170817 and γ-ray burst GRB 170817A associated with a galaxy at a distance of 40 megaparsecs from Earth are described.
Abstract: The merger of two neutron stars is predicted to give rise to three major detectable phenomena: a short burst of gamma-rays, a gravitational wave signal, and a transient optical/near-infrared source powered by the synthesis of large amounts of very heavy elements via rapid neutron capture (the r-process). Such transients, named "macronovae" or "kilonovae", are believed to be centres of production of rare elements such as gold and platinum. The most compelling evidence so far for a kilonova was a very faint near-infrared rebrightening in the afterglow of a short gamma-ray burst at z = 0.356, although findings indicating bluer events have been reported. Here we report the spectral identification and describe the physical properties of a bright kilonova associated with the gravitational wave source GW 170817 and gamma-ray burst GRB 170817A associated with a galaxy at a distance of 40 Mpc from Earth. Using a series of spectra from ground-based observatories covering the wavelength range from the ultraviolet to the near-infrared, we find that the kilonova is characterized by rapidly expanding ejecta with spectral features similar to those predicted by current models. The ejecta is optically thick early on, with a velocity of about 0.2 times light speed, and reaches a radius of about 50 astronomical units in only 1.5 days. As the ejecta expands, broad absorption-like lines appear on the spectral continuum indicating atomic species produced by nucleosynthesis that occurs in the post-merger fast-moving dynamical ejecta and in two slower (0.05 times light speed) wind regions. Comparison with spectral models suggests that the merger ejected 0.03-0.05 solar masses of material, including high-opacity lanthanides.

771 citations


Journal ArticleDOI
TL;DR: Experts assembled to review, debate and summarize the challenges of IB validation and qualification produced 14 key recommendations for accelerating the clinical translation of IBs, which highlight the role of parallel (rather than sequential) tracks of technical validation, biological/clinical validation and assessment of cost-effectiveness.
Abstract: Imaging biomarkers (IBs) are integral to the routine management of patients with cancer. IBs used daily in oncology include clinical TNM stage, objective response and left ventricular ejection fraction. Other CT, MRI, PET and ultrasonography biomarkers are used extensively in cancer research and drug development. New IBs need to be established either as useful tools for testing research hypotheses in clinical trials and research studies, or as clinical decision-making tools for use in healthcare, by crossing 'translational gaps' through validation and qualification. Important differences exist between IBs and biospecimen-derived biomarkers and, therefore, the development of IBs requires a tailored 'roadmap'. Recognizing this need, Cancer Research UK (CRUK) and the European Organisation for Research and Treatment of Cancer (EORTC) assembled experts to review, debate and summarize the challenges of IB validation and qualification. This consensus group has produced 14 key recommendations for accelerating the clinical translation of IBs, which highlight the role of parallel (rather than sequential) tracks of technical (assay) validation, biological/clinical validation and assessment of cost-effectiveness; the need for IB standardization and accreditation systems; the need to continually revisit IB precision; an alternative framework for biological/clinical validation of IBs; and the essential requirements for multicentre studies to qualify IBs for clinical use.

758 citations


Journal ArticleDOI
TL;DR: This update of a previously published Cochrane review sought to critically appraise and summarise current evidence on the effectiveness and resource use of CGA for older adults admitted to hospital, and to estimate its cost-effectiveness.
Abstract: Background Comprehensive geriatric assessment (CGA) is a multi-dimensional, multi-disciplinary diagnostic and therapeutic process conducted to determine the medical, mental, and functional problems of older people with frailty so that a co-ordinated and integrated plan for treatment and follow-up can be developed. This is an update of a previously published Cochrane review. Objectives We sought to critically appraise and summarise current evidence on the effectiveness and resource use of CGA for older adults admitted to hospital, and to use these data to estimate its cost-effectiveness. Search methods We searched CENTRAL, MEDLINE, Embase, three other databases, and two trials registers on 5 October 2016; we also checked reference lists and contacted study authors. Selection criteria We included randomised trials that compared inpatient CGA (delivered on geriatric wards or by mobile teams) versus usual care on a general medical ward or on a ward for older people, usually admitted to hospital for acute care or for inpatient rehabilitation after an acute admission. Data collection and analysis We followed standard methodological procedures expected by Cochrane and Effective Practice and Organisation of Care (EPOC). We used the GRADE approach to assess the certainty of evidence for the most important outcomes. For this update, we requested individual patient data (IPD) from trialists, and we conducted a survey of trialists to obtain details of delivery of CGA. We calculated risk ratios (RRs), mean differences (MDs), or standardised mean differences (SMDs), and combined data using fixed-effect meta-analysis. We estimated cost-effectiveness by comparing inpatient CGA versus hospital admission without CGA in terms of cost per quality-adjusted life year (QALY) gained, cost per life year (LY) gained, and cost per life year living at home (LYLAH) gained. Main results We included 29 trials recruiting 13,766 participants across nine, mostly high-income countries. CGA increases the likelihood that patients will be alive and in their own homes at 3 to 12 months' follow-up (risk ratio (RR) 1.06, 95% confidence interval (CI) 1.01 to 1.10; 16 trials, 6799 participants; high-certainty evidence), results in little or no difference in mortality at 3 to 12 months' follow-up (RR 1.00, 95% CI 0.93 to 1.07; 21 trials, 10,023 participants; high-certainty evidence), decreases the likelihood that patients will be admitted to a nursing home at 3 to 12 months follow-up (RR 0.80, 95% CI 0.72 to 0.89; 14 trials, 6285 participants; high-certainty evidence) and results in little or no difference in dependence (RR 0.97, 95% CI 0.89 to 1.04; 14 trials, 6551 participants; high-certainty evidence). CGA may make little or no difference to cognitive function (SMD ranged from -0.22 to 0.35 (5 trials, 3534 participants; low-certainty evidence)). Mean length of stay ranged from 1.63 days to 40.7 days in the intervention group, and ranged from 1.8 days to 42.8 days in the comparison group. Healthcare costs per participant in the CGA group were on average GBP 234 (95% CI GBP -144 to GBP 605) higher than in the usual care group (17 trials, 5303 participants; low-certainty evidence). CGA may lead to a slight increase in QALYs of 0.012 (95% CI -0.024 to 0.048) at GBP 19,802 per QALY gained (3 trials; low-certainty evidence), a slight increase in LYs of 0.037 (95% CI 0.001 to 0.073), at GBP 6305 per LY gained (4 trials; low-certainty evidence), and a slight increase in LYLAH of 0.019 (95% CI -0.019 to 0.155) at GBP 12,568 per LYLAH gained (2 trials; low-certainty evidence). The probability that CGA would be cost-effective at a GBP 20,000 ceiling ratio for QALY, LY, and LYLAH was 0.50, 0.89, and 0.47, respectively (17 trials, 5303 participants; low-certainty evidence). Authors' conclusions Older patients are more likely to be alive and in their own homes at follow-up if they received CGA on admission to hospital. We are uncertain whether data show a difference in effect between wards and teams, as this analysis was underpowered. CGA may lead to a small increase in costs, and evidence for cost-effectiveness is of low-certainty due to imprecision and inconsistency among studies. Further research that reports cost estimates that are setting-specific across different sectors of care are required.

758 citations


Journal ArticleDOI
TL;DR: This paper surveys research on ensembles for data stream classification as well as regression tasks and discusses advanced learning concepts such as imbalanced data streams, novelty detection, active and semi-supervised learning, complex data representations and structured outputs.

757 citations


Journal ArticleDOI
Rebecca Sims1, Sven J. van der Lee2, Adam C. Naj3, Céline Bellenguez4  +484 moreInstitutions (120)
TL;DR: Three new genome-wide significant nonsynonymous variants associated with Alzheimer's disease are observed, providing additional evidence that the microglia-mediated innate immune response contributes directly to the development of Alzheimer's Disease.
Abstract: We identified rare coding variants associated with Alzheimer's disease in a three-stage case–control study of 85,133 subjects. In stage 1, we genotyped 34,174 samples using a whole-exome microarray. In stage 2, we tested associated variants (P < 1 × 10−4) in 35,962 independent samples using de novo genotyping and imputed genotypes. In stage 3, we used an additional 14,997 samples to test the most significant stage 2 associations (P < 5 × 10−8) using imputed genotypes. We observed three new genome-wide significant nonsynonymous variants associated with Alzheimer's disease: a protective variant in PLCG2 (rs72824905: p.Pro522Arg, P = 5.38 × 10−10, odds ratio (OR) = 0.68, minor allele frequency (MAF)cases = 0.0059, MAFcontrols = 0.0093), a risk variant in ABI3 (rs616338: p.Ser209Phe, P = 4.56 × 10−10, OR = 1.43, MAFcases = 0.011, MAFcontrols = 0.008), and a new genome-wide significant variant in TREM2 (rs143332484: p.Arg62His, P = 1.55 × 10−14, OR = 1.67, MAFcases = 0.0143, MAFcontrols = 0.0089), a known susceptibility gene for Alzheimer's disease. These protein-altering changes are in genes highly expressed in microglia and highlight an immune-related protein–protein interaction network enriched for previously identified risk genes in Alzheimer's disease. These genetic findings provide additional evidence that the microglia-mediated innate immune response contributes directly to the development of Alzheimer's disease.

Journal ArticleDOI
TL;DR: How established methods of meta‐regression and random effects modelling from mainstream meta‐analysis are being adapted to perform MR analyses are clarified, and the ability of two popular random effects models to provide robustness to pleiotropy under the IVW approach is investigated.
Abstract: Mendelian randomization (MR) uses genetic data to probe questions of causality in epidemiological research, by invoking the Instrumental Variable (IV) assumptions. In recent years, it has become commonplace to attempt MR analyses by synthesising summary data estimates of genetic association gleaned from large and independent study populations. This is referred to as two-sample summary data MR. Unfortunately, due to the sheer number of variants that can be easily included into summary data MR analyses, it is increasingly likely that some do not meet the IV assumptions due to pleiotropy. There is a pressing need to develop methods that can both detect and correct for pleiotropy, in order to preserve the validity of the MR approach in this context. In this paper, we aim to clarify how established methods of meta-regression and random effects modelling from mainstream meta-analysis are being adapted to perform this task. Specifically, we focus on two contrastin g approaches: the Inverse Variance Weighted (IVW) method which assumes in its simplest form that all genetic variants are valid IVs, and the method of MR-Egger regression that allows all variants to violate the IV assumptions, albeit in a specific way. We investigate the ability of two popular random effects models to provide robustness to pleiotropy under the IVW approach, and propose statistics to quantify the relative goodness-of-fit of the IVW approach over MR-Egger regression. © 2017 The Authors. Statistics in Medicine Published by JohnWiley & Sons Ltd.


Journal ArticleDOI
TL;DR: In this article, the authors reported the discovery and monitoring of the near-infrared counterpart (AT2017gfo) of a binary neutron-star merger event detected as a gravitational wave source by Advanced Laser Interferometer Gravitational-wave Observatory (LIGO)/Virgo (GW170817) and as a short gamma-ray burst by Fermi Gamma-ray Burst Monitor (GBM) and Integral SPI-ACS (GRB 170817A).
Abstract: We report the discovery and monitoring of the near-infrared counterpart (AT2017gfo) of a binary neutron-star merger event detected as a gravitational wave source by Advanced Laser Interferometer Gravitational-wave Observatory (LIGO)/Virgo (GW170817) and as a short gamma-ray burst by Fermi Gamma-ray Burst Monitor (GBM) and Integral SPI-ACS (GRB 170817A). The evolution of the transient light is consistent with predictions for the behavior of a "kilonova/macronova" powered by the radioactive decay of massive neutron-rich nuclides created via r-process nucleosynthesis in the neutron-star ejecta. In particular, evidence for this scenario is found from broad features seen in Hubble Space Telescope infrared spectroscopy, similar to those predicted for lanthanide-dominated ejecta, and the much slower evolution in the near-infrared ${K}_{{\rm{s}}}$-band compared to the optical. This indicates that the late-time light is dominated by high-opacity lanthanide-rich ejecta, suggesting nucleosynthesis to the third r-process peak (atomic masses $A\approx 195$). This discovery confirms that neutron-star mergers produce kilo-/macronovae and that they are at least a major—if not the dominant—site of rapid neutron capture nucleosynthesis in the universe.

Journal ArticleDOI
Mansi M. Kasliwal1, Ehud Nakar2, Leo Singer3, Leo Singer4, David L. Kaplan5, David O. Cook1, A. Van Sistine5, R. M. Lau1, Christoffer Fremling1, Ore Gottlieb2, Jacob E. Jencson1, Scott M. Adams1, U. Feindt6, Kenta Hotokezaka7, Sourav Ghosh5, Daniel A. Perley8, Po-Chieh Yu9, Tsvi Piran10, James R. Allison11, James R. Allison12, G. C. Anupama13, Arvind Balasubramanian14, Keith W. Bannister15, John Bally16, Jennifer Barnes17, Sudhanshu Barway, Eric C. Bellm18, Varun Bhalerao19, Deb Sankar Bhattacharya20, Nadejda Blagorodnova1, Joshua S. Bloom21, Joshua S. Bloom22, Patrick Brady5, Chris Cannella1, Deep Chatterjee5, S. B. Cenko4, S. B. Cenko3, B. E. Cobb23, Chris M. Copperwheat8, A. Corsi24, Kaushik De1, Dougal Dobie12, Dougal Dobie15, Dougal Dobie11, S. W. K. Emery25, Phil Evans26, Ori D. Fox27, Dale A. Frail28, C. Frohmaier29, C. Frohmaier30, Ariel Goobar6, Gregg Hallinan1, Fiona A. Harrison1, George Helou1, Tanja Hinderer31, Anna Y. Q. Ho1, Assaf Horesh10, Wing-Huen Ip7, Ryosuke Itoh32, Daniel Kasen22, Hyesook Kim, N. P. M. Kuin25, Thomas Kupfer1, Christene Lynch12, Christene Lynch11, K. K. Madsen1, Paolo A. Mazzali8, Paolo A. Mazzali33, Adam A. Miller34, Adam A. Miller35, Kunal Mooley36, Tara Murphy12, Tara Murphy11, Chow-Choong Ngeow9, David A. Nichols31, Samaya Nissanke31, Peter Nugent22, Peter Nugent21, Eran O. Ofek37, H. Qi5, Robert M. Quimby38, Robert M. Quimby39, Stephan Rosswog6, Florin Rusu40, Elaine M. Sadler12, Elaine M. Sadler11, Patricia Schmidt31, Jesper Sollerman6, Iain A. Steele8, A. R. Williamson31, Y. Xu1, Lin Yan1, Yoichi Yatsu32, C. Zhang5, Weijie Zhao40 
22 Dec 2017-Science
TL;DR: It is demonstrated that merging neutron stars are a long-sought production site forging heavy elements by r-process nucleosynthesis, which is dissimilar to classical short gamma-ray bursts with ultrarelativistic jets.
Abstract: Merging neutron stars offer an excellent laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart (EM170817) with gravitational waves (GW170817) detected from merging neutron stars. By synthesizing a panchromatic data set, we demonstrate that merging neutron stars are a long-sought production site forging heavy elements by r-process nucleosynthesis. The weak gamma rays seen in EM170817 are dissimilar to classical short gamma-ray bursts with ultrarelativistic jets. Instead, we suggest that breakout of a wide-angle, mildly relativistic cocoon engulfing the jet explains the low-luminosity gamma rays, the high-luminosity ultraviolet-optical-infrared, and the delayed radio and x-ray emission. We posit that all neutron star mergers may lead to a wide-angle cocoon breakout, sometimes accompanied by a successful jet and sometimes by a choked jet.

Journal ArticleDOI
TL;DR: Treatment with SGLT-2i versus other glucose-lowering drugs was associated with a lower risk of HHF and death, suggesting that the benefits seen with empagliflozin in a randomized trial may be a class effect applicable to a broad population of patients with type 2 diabetes mellitus in real-world practice.
Abstract: Background:Reduction in cardiovascular death and hospitalization for heart failure (HHF) was recently reported with the sodium-glucose cotransporter-2 inhibitor (SGLT-2i) empagliflozin in patients ...

Journal ArticleDOI
Christopher P. Nelson1, Christopher P. Nelson2, Anuj Goel3, Anuj Goel4, Adam S. Butterworth5, Stavroula Kanoni6, Tom R. Webb1, Tom R. Webb2, Eirini Marouli6, Lingyao Zeng7, Ioanna Ntalla6, Florence Lai2, Florence Lai1, Jemma C. Hopewell4, Olga Giannakopoulou6, Tao Jiang5, Stephen E. Hamby1, Stephen E. Hamby2, Emanuele Di Angelantonio5, Themistocles L. Assimes8, Erwin P. Bottinger9, John C. Chambers10, John C. Chambers11, John C. Chambers12, Robert Clarke4, Colin N. A. Palmer13, Richard M Cubbon14, Patrick T. Ellinor15, Raili Ermel16, Evangelos Evangelou12, Evangelos Evangelou17, Paul W. Franks18, Paul W. Franks19, Paul W. Franks20, Christopher Grace4, Christopher Grace3, Dongfeng Gu21, Aroon D. Hingorani22, Joanna M. M. Howson5, Erik Ingelsson8, Adnan Kastrati7, Thorsten Kessler7, Theodosios Kyriakou4, Theodosios Kyriakou3, Terho Lehtimäki23, Xiangfeng Lu8, Yingchang Lu9, Yingchang Lu24, Winfried März25, Winfried März26, Winfried März27, Ruth McPherson28, Andres Metspalu29, Mar Pujades-Rodriguez14, Arno Ruusalepp16, Eric E. Schadt9, Amand F. Schmidt22, Michael J. Sweeting5, Pierre Zalloua30, Pierre Zalloua20, Kamal Alghalayini31, Bernard Keavney32, Bernard Keavney33, Jaspal S. Kooner34, Jaspal S. Kooner10, Jaspal S. Kooner11, Ruth J. F. Loos9, Riyaz S. Patel35, Martin K. Rutter33, Martin K. Rutter32, Maciej Tomaszewski33, Maciej Tomaszewski36, Ioanna Tzoulaki12, Ioanna Tzoulaki17, Eleftheria Zeggini37, Jeanette Erdmann38, George Dedoussis39, Johan L.M. Björkegren9, Johan L.M. Björkegren40, CARDIoGRAMplusC D4, Heribert Schunkert7, Martin Farrall3, Martin Farrall4, John Danesh37, John Danesh5, Nilesh J. Samani1, Nilesh J. Samani2, Hugh Watkins3, Hugh Watkins4, Panos Deloukas31, Panos Deloukas6 
TL;DR: This approach identified 13 new loci at genome-wide significance, 12 of which were on the previous list of loci meeting the 5% FDR threshold, thus providing strong support that the remaining loci identified by FDR represent genuine signals.
Abstract: Genome-wide association studies (GWAS) in coronary artery disease (CAD) had identified 66 loci at 'genome-wide significance' (P < 5 × 10-8) at the time of this analysis, but a much larger number of putative loci at a false discovery rate (FDR) of 5% (refs. 1,2,3,4). Here we leverage an interim release of UK Biobank (UKBB) data to evaluate the validity of the FDR approach. We tested a CAD phenotype inclusive of angina (SOFT; ncases = 10,801) as well as a stricter definition without angina (HARD; ncases = 6,482) and selected cases with the former phenotype to conduct a meta-analysis using the two most recent CAD GWAS. This approach identified 13 new loci at genome-wide significance, 12 of which were on our previous list of loci meeting the 5% FDR threshold, thus providing strong support that the remaining loci identified by FDR represent genuine signals. The 304 independent variants associated at 5% FDR in this study explain 21.2% of CAD heritability and identify 243 loci that implicate pathways in blood vessel morphogenesis as well as lipid metabolism, nitric oxide signaling and inflammation.

Journal ArticleDOI
Dajiang J. Liu1, Gina M. Peloso2, Gina M. Peloso3, Haojie Yu4  +285 moreInstitutions (91)
TL;DR: It is found that beta-thalassemia trait carriers displayed lower TC and were protected from coronary artery disease (CAD), and only some mechanisms of lowering LDL-C appeared to increase risk for type 2 diabetes (T2D); and TG-lowering alleles involved in hepatic production of TG-rich lipoproteins tracked with higher liver fat, higher risk for T2D, and lower risk for CAD.
Abstract: We screened variants on an exome-focused genotyping array in >300,000 participants (replication in >280,000 participants) and identified 444 independent variants in 250 loci significantly associated with total cholesterol (TC), high-density-lipoprotein cholesterol (HDL-C), low-density-lipoprotein cholesterol (LDL-C), and/or triglycerides (TG). At two loci (JAK2 and A1CF), experimental analysis in mice showed lipid changes consistent with the human data. We also found that: (i) beta-thalassemia trait carriers displayed lower TC and were protected from coronary artery disease (CAD); (ii) excluding the CETP locus, there was not a predictable relationship between plasma HDL-C and risk for age-related macular degeneration; (iii) only some mechanisms of lowering LDL-C appeared to increase risk for type 2 diabetes (T2D); and (iv) TG-lowering alleles involved in hepatic production of TG-rich lipoproteins (TM6SF2 and PNPLA3) tracked with higher liver fat, higher risk for T2D, and lower risk for CAD, whereas TG-lowering alleles involved in peripheral lipolysis (LPL and ANGPTL4) had no effect on liver fat but decreased risks for both T2D and CAD.

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TL;DR: In this paper, the authors report genetic association of blood pressure (systolic, diastolic, pulse pressure) among UK Biobank participants of European ancestry with independent replication in other cohorts, and robust validation of 107 independent loci.
Abstract: Elevated blood pressure is the leading heritable risk factor for cardiovascular disease worldwide. We report genetic association of blood pressure (systolic, diastolic, pulse pressure) among UK Biobank participants of European ancestry with independent replication in other cohorts, and robust validation of 107 independent loci. We also identify new independent variants at 11 previously reported blood pressure loci. In combination with results from a range of in silico functional analyses and wet bench experiments, our findings highlight new biological pathways for blood pressure regulation enriched for genes expressed in vascular tissues and identify potential therapeutic targets for hypertension. Results from genetic risk score models raise the possibility of a precision medicine approach through early lifestyle intervention to offset the impact of blood pressure-raising genetic variants on future cardiovascular disease risk.

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TL;DR: A comprehensive summary of the current state of knowledge of zinc-finger proteins, their structure and functions is provided and the biological role of ZNFs in the development of organisms under normal physiological and pathological conditions is focused on.
Abstract: Zinc-finger proteins (ZNFs) are one of the most abundant groups of proteins and have a wide range of molecular functions. Given the wide variety of zinc-finger domains, ZNFs are able to interact with DNA, RNA, PAR (poly-ADP-ribose) and other proteins. Thus, ZNFs are involved in the regulation of several cellular processes. In fact, ZNFs are implicated in transcriptional regulation, ubiquitin-mediated protein degradation, signal transduction, actin targeting, DNA repair, cell migration, and numerous other processes. The aim of this review is to provide a comprehensive summary of the current state of knowledge of this class of proteins. Firstly, we describe the actual classification of ZNFs, their structure and functions. Secondly, we focus on the biological role of ZNFs in the development of organisms under normal physiological and pathological conditions.

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02 Feb 2017-Nature
TL;DR: Radiocarbon dates indicate that peat began accumulating from about 10,600 years ago, coincident with the onset of more humid conditions in central Africa at the beginning of the Holocene, making the Cuvette Centrale depression in the central Congo Basin the most extensive peatland complex in the tropics.
Abstract: Peatlands are carbon-rich ecosystems that cover just three per cent of Earth's land surface, but store one-third of soil carbon. Peat soils are formed by the build-up of partially decomposed organic matter under waterlogged anoxic conditions. Most peat is found in cool climatic regions where unimpeded decomposition is slower, but deposits are also found under some tropical swamp forests. Here we present field measurements from one of the world's most extensive regions of swamp forest, the Cuvette Centrale depression in the central Congo Basin. We find extensive peat deposits beneath the swamp forest vegetation (peat defined as material with an organic matter content of at least 65 per cent to a depth of at least 0.3 metres). Radiocarbon dates indicate that peat began accumulating from about 10,600 years ago, coincident with the onset of more humid conditions in central Africa at the beginning of the Holocene. The peatlands occupy large interfluvial basins, and seem to be largely rain-fed and ombrotrophic-like (of low nutrient status) systems. Although the peat layer is relatively shallow (with a maximum depth of 5.9 metres and a median depth of 2.0 metres), by combining in situ and remotely sensed data, we estimate the area of peat to be approximately 145,500 square kilometres (95 per cent confidence interval of 131,900-156,400 square kilometres), making the Cuvette Centrale the most extensive peatland complex in the tropics. This area is more than five times the maximum possible area reported for the Congo Basin in a recent synthesis of pantropical peat extent. We estimate that the peatlands store approximately 30.6 petagrams (30.6 × 10(15) grams) of carbon belowground (95 per cent confidence interval of 6.3-46.8 petagrams of carbon)-a quantity that is similar to the above-ground carbon stocks of the tropical forests of the entire Congo Basin. Our result for the Cuvette Centrale increases the best estimate of global tropical peatland carbon stocks by 36 per cent, to 104.7 petagrams of carbon (minimum estimate of 69.6 petagrams of carbon; maximum estimate of 129.8 petagrams of carbon). This stored carbon is vulnerable to land-use change and any future reduction in precipitation.

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TL;DR: There is strong evidence that insomnia is a causal factor in the occurrence of psychotic experiences and other mental health problems, and the treatment of disrupted sleep might require a higher priority in mental health provision.

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24 Feb 2017-Science
TL;DR: Observations showing that NGC 5907 ULX is instead an x-ray accreting neutron star (NS) with a spin period evolving from 1.43 seconds in 2003 to 1.13 seconds in 2014 suggest that other extreme ULXs (x-ray luminosity ≥ 1041 erg second−1) might harbor NSs.
Abstract: Ultraluminous x-ray sources (ULXs) in nearby galaxies shine brighter than any x-ray source in our Galaxy. ULXs are usually modeled as stellar-mass black holes (BHs) accreting at very high rates or intermediate-mass BHs. We present observations showing that NGC 5907 ULX is instead an x-ray accreting neutron star (NS) with a spin period evolving from 1.43 seconds in 2003 to 1.13 seconds in 2014. It has an isotropic peak luminosity of ~1000 times the Eddington limit for a NS at 17.1 megaparsec. Standard accretion models fail to explain its luminosity, even assuming beamed emission, but a strong multipolar magnetic field can describe its properties. These findings suggest that other extreme ULXs (x-ray luminosity ≥ 1041 erg second−1) might harbor NSs.

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TL;DR: In this paper, the authors assess the assumption that more and more work is being detached from place and that this is a "win-win" for both employers and employees, and they find that only one-third of the increase in remote working can be explained by compositional factors such as movement to the knowledge economy, the growth in flexible employment and organisational responses to the changing demographic make-up of the employed labour force.
Abstract: This paper critically assesses the assumption that more and more work is being detached from place and that this is a ‘win-win’ for both employers and employees. Based on an analysis of official labour market data, it finds that only one-third of the increase in remote working can be explained by compositional factors such as movement to the knowledge economy, the growth in flexible employment and organisational responses to the changing demographic make-up of the employed labour force. This suggests that the detachment of work from place is a growing trend. The paper also shows that while remote working is associated with higher organisational commitment, job satisfaction and job-related well-being, these benefits come at the cost of work intensification and a greater inability to switch off.

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James D. McKay1, Rayjean J. Hung2, Younghun Han3, Xuchen Zong2, Robert Carreras-Torres1, David C. Christiani4, Neil E. Caporaso5, Mattias Johansson1, Xiangjun Xiao3, Yafang Li3, Jinyoung Byun3, Alison M. Dunning6, Karen A. Pooley6, David C. Qian3, Xuemei Ji3, Geoffrey Liu2, Maria Timofeeva1, Stig E. Bojesen7, Stig E. Bojesen8, Stig E. Bojesen9, Xifeng Wu10, Loic Le Marchand11, Demetrios Albanes5, Heike Bickeböller12, Melinda C. Aldrich13, William S. Bush14, Adonina Tardón15, Gad Rennert16, M. Dawn Teare17, John K. Field18, Lambertus A. Kiemeney19, Philip Lazarus20, Aage Haugen21, Stephen Lam22, Matthew B. Schabath, Angeline S. Andrew3, Hongbing Shen23, Yun Chul Hong24, Jian-Min Yuan25, Pier Alberto Bertazzi26, Angela Cecilia Pesatori26, Yuanqing Ye10, Nancy Diao4, Li Su4, Ruyang Zhang4, Yonathan Brhane2, Natasha B. Leighl27, Jakob S Johansen9, Anders Mellemgaard9, Walid Saliba16, Christopher A. Haiman28, Lynne R. Wilkens11, Ana Fernández-Somoano15, Guillermo Fernández-Tardón15, Henricus F. M. van der Heijden19, Jin Hee Kim29, Juncheng Dai23, Zhibin Hu23, Michael P.A. Davies18, Michael W. Marcus18, Hans Brunnström30, Jonas Manjer30, Olle Melander30, David C. Muller31, Kim Overvad32, Antonia Trichopoulou, Rosario Tumino33, Jennifer A. Doherty, Matt P Barnett34, Chu Chen34, Gary E. Goodman, Angela Cox17, Fiona Taylor17, Penella J. Woll17, Irene Brüske, H-Erich Wichmann35, H-Erich Wichmann36, Judith Manz, Thomas Muley37, Angela Risch, Albert Rosenberger12, Kjell Grankvist38, Mikael Johansson38, Frances A. Shepherd27, Ming-Sound Tsao27, Susanne M. Arnold39, Eric B. Haura, Ciprian Bolca, Ivana Holcatova40, Vladimir Janout41, Milica Kontic42, Jolanta Lissowska, Anush Mukeria, Simona Ognjanovic, Tadeusz M Orlowski, Ghislaine Scelo1, Beata Swiatkowska43, David Zaridze, Per Bakke44, Vidar Skaug21, Shanbeh Zienolddiny21, Eric J. Duell, Lesley M. Butler25, Woon-Puay Koh45, Yu-Tang Gao, Richard S. Houlston46, John McLaughlin, Victoria L. Stevens47, Philippe Joubert, Maxime Lamontagne, David C. Nickle48, Ma'en Obeidat49, Wim Timens50, Bin Zhu5, Lei Song5, Linda Kachuri2, María Soler Artigas51, María Soler Artigas52, Martin D. Tobin52, Martin D. Tobin51, Louise V. Wain51, Louise V. Wain52, Thorunn Rafnar53, Thorgeir E. Thorgeirsson53, Gunnar W Reginsson53, Kari Stefansson53, Dana B. Hancock54, Laura J. Bierut55, Margaret R. Spitz56, Nathan C. Gaddis54, Sharon M. Lutz57, Fangyi Gu5, Eric O. Johnson54, Ahsan Kamal3, Claudio W. Pikielny3, Dakai Zhu3, Sara Lindstroem58, Xia Jiang4, Rachel F. Tyndale59, Rachel F. Tyndale60, Georgia Chenevix-Trench61, Jonathan Beesley61, Yohan Bossé62, Stephen J. Chanock5, Paul Brennan1, Maria Teresa Landi5, Christopher I. Amos3 
International Agency for Research on Cancer1, Lunenfeld-Tanenbaum Research Institute2, Dartmouth College3, Harvard University4, National Institutes of Health5, University of Cambridge6, Gentofte Hospital7, University of Copenhagen8, Copenhagen University Hospital9, University of Texas MD Anderson Cancer Center10, University of Hawaii11, University of Göttingen12, Vanderbilt University Medical Center13, Case Western Reserve University14, University of Oviedo15, Technion – Israel Institute of Technology16, University of Sheffield17, University of Liverpool18, Radboud University Nijmegen19, Washington State University Spokane20, National Institute of Occupational Health21, BC Cancer Agency22, Nanjing Medical University23, New Generation University College24, University of Pittsburgh25, University of Milan26, Princess Margaret Cancer Centre27, University of Southern California28, Sejong University29, Lund University30, Imperial College London31, Aarhus University32, Prevention Institute33, Fred Hutchinson Cancer Research Center34, Ludwig Maximilian University of Munich35, Technische Universität München36, University Hospital Heidelberg37, Umeå University38, University of Kentucky39, Charles University in Prague40, University of Ostrava41, University of Belgrade42, Nofer Institute of Occupational Medicine43, University of Bergen44, National University of Singapore45, Institute of Cancer Research46, American Cancer Society47, Merck & Co.48, University of British Columbia49, University Medical Center Groningen50, National Institute for Health Research51, University of Leicester52, Amgen53, Research Triangle Park54, Washington University in St. Louis55, Baylor College of Medicine56, Anschutz Medical Campus57, University of Washington58, Centre for Addiction and Mental Health59, University of Toronto60, QIMR Berghofer Medical Research Institute61, Laval University62
TL;DR: 18 susceptibility loci achieving genome-wide significance are identified, including 10 new loci linked with lung cancer overall and six loci associated with lung adenocarcinoma, highlighting the striking heterogeneity in genetic susceptibility across the histological subtypes of lung cancer.
Abstract: Although several lung cancer susceptibility loci have been identified, much of the heritability for lung cancer remains unexplained. Here 14,803 cases and 12,262 controls of European descent were genotyped on the OncoArray and combined with existing data for an aggregated genome-wide association study (GWAS) analysis of lung cancer in 29,266 cases and 56,450 controls. We identified 18 susceptibility loci achieving genome-wide significance, including 10 new loci. The new loci highlight the striking heterogeneity in genetic susceptibility across the histological subtypes of lung cancer, with four loci associated with lung cancer overall and six loci associated with lung adenocarcinoma. Gene expression quantitative trait locus (eQTL) analysis in 1,425 normal lung tissue samples highlights RNASET2, SECISBP2L and NRG1 as candidate genes. Other loci include genes such as a cholinergic nicotinic receptor, CHRNA2, and the telomere-related genes OFBC1 and RTEL1. Further exploration of the target genes will continue to provide new insights into the etiology of lung cancer.

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TL;DR: This review outlines the understanding of carboxylate-assisted C-H activation in terms of the "ambiphilic metal-ligand assistance" and "concerted metalation deprotonation" concepts and some opportunities where the interplay between computation and experiment may contribute further to the areas of catalytic C- H functionalization and applied computational chemistry are identified.
Abstract: Computational studies on carboxylate-assisted C–H activation and functionalization at group 8–10 transition metal centers are reviewed This Review is organized by metal and will cover work published from late 2009 until mid-2016 A brief overview of computational work prior to 2010 is also provided, and this outlines the understanding of carboxylate-assisted C–H activation in terms of the “ambiphilic metal–ligand assistance” (AMLA) and “concerted metalation deprotonation” (CMD) concepts Computational studies are then surveyed in terms of the nature of the C–H bond being activated (C(sp2)–H or C(sp3)–H), the nature of the process involved (intramolecular with a directing group or intermolecular), and the context (stoichiometric C–H activation or within a variety of catalytic processes) This Review aims to emphasize the connection between computation and experiment and to highlight the contribution of computational chemistry to our understanding of catalytic C–H functionalization based on carboxylate-ass

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Mansi M. Kasliwal1, Ehud Nakar2, Leo Singer3, Leo Singer4, David L. Kaplan5, David O. Cook1, A. Van Sistine5, R. M. Lau1, Christoffer Fremling1, Ore Gottlieb2, Jacob E. Jencson1, Scott M. Adams1, U. Feindt6, Kenta Hotokezaka7, Sourav Ghosh5, Daniel A. Perley8, Po-Chieh Yu9, Tsvi Piran10, James R. Allison11, James R. Allison12, G. C. Anupama13, Arvind Balasubramanian14, Keith W. Bannister15, John Bally16, Jennifer Barnes17, Sudhanshu Barway, Eric C. Bellm18, Varun Bhalerao19, Deb Sankar Bhattacharya20, Nadejda Blagorodnova1, Joshua S. Bloom21, Joshua S. Bloom22, Patrick Brady5, Chris Cannella1, Deep Chatterjee5, S. B. Cenko4, S. B. Cenko3, B. E. Cobb23, Chris M. Copperwheat8, A. Corsi24, Kaushik De1, Dougal Dobie11, Dougal Dobie15, Dougal Dobie12, S. W. K. Emery25, Phil Evans26, Ori D. Fox27, Dale A. Frail28, C. Frohmaier29, C. Frohmaier30, Ariel Goobar6, Gregg Hallinan1, Fiona A. Harrison1, George Helou1, Tanja Hinderer31, Anna Y. Q. Ho1, Assaf Horesh10, Wing-Huen Ip7, Ryosuke Itoh32, Daniel Kasen22, Hyesook Kim, N. P. M. Kuin25, Thomas Kupfer1, Christene Lynch12, Christene Lynch11, K. K. Madsen1, Paolo A. Mazzali33, Paolo A. Mazzali8, Adam A. Miller34, Adam A. Miller35, Kunal Mooley36, Tara Murphy12, Tara Murphy11, Chow-Choong Ngeow9, David A. Nichols31, Samaya Nissanke31, Peter Nugent21, Peter Nugent22, Eran O. Ofek37, H. Qi5, Robert M. Quimby38, Robert M. Quimby39, Stephan Rosswog6, Florin Rusu40, Elaine M. Sadler11, Elaine M. Sadler12, Patricia Schmidt31, Jesper Sollerman6, Iain A. Steele8, A. R. Williamson31, Y. Xu1, Lin Yan1, Yoichi Yatsu32, C. Zhang5, Weijie Zhao40 
TL;DR: In this paper, the authors established the physical association of an electromagnetic counterpart EM170817 to gravitational waves (GW 170817) detected from merging neutron stars by synthesizing a panchromatic dataset.
Abstract: Merging neutron stars offer an exquisite laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart EM170817 to gravitational waves (GW170817) detected from merging neutron stars. By synthesizing a panchromatic dataset, we demonstrate that merging neutron stars are a long-sought production site forging heavy elements by r-process nucleosynthesis. The weak gamma-rays seen in EM170817 are dissimilar to classical short gamma-ray bursts with ultra-relativistic jets. Instead, we suggest that breakout of a wide-angle, mildly-relativistic cocoon engulfing the jet elegantly explains the low-luminosity gamma-rays, the high-luminosity ultraviolet-optical-infrared and the delayed radio/X-ray emission. We posit that all merging neutron stars may lead to a wide-angle cocoon breakout; sometimes accompanied by a successful jet and sometimes a choked jet.

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TL;DR: In this meta‐analysis of individual patient data, EGDT did not result in better outcomes than usual care and was associated with higher hospitalization costs across a broad range of patient and hospital characteristics.
Abstract: BACKGROUND: After a single-center trial and observational studies suggesting that early, goal-directed therapy (EGDT) reduced mortality from septic shock, three multicenter trials (ProCESS, ARISE, and ProMISe) showed no benefit. This meta-analysis of individual patient data from the three recent trials was designed prospectively to improve statistical power and explore heterogeneity of treatment effect of EGDT. METHODS: We harmonized entry criteria, intervention protocols, outcomes, resource-use measures, and data collection across the trials and specified all analyses before unblinding. After completion of the trials, we pooled data, excluding the protocol-based standard-therapy group from the ProCESS trial, and resolved residual differences. The primary outcome was 90-day mortality. Secondary outcomes included 1-year survival, organ support, and hospitalization costs. We tested for treatment-by-subgroup interactions for 16 patient characteristics and 6 care-delivery characteristics. RESULTS: We studied 3723 patients at 138 hospitals in seven countries. Mortality at 90 days was similar for EGDT (462 of 1852 patients [24.9%]) and usual care (475 of 1871 patients [25.4%]); the adjusted odds ratio was 0.97 (95% confidence interval, 0.82 to 1.14; P=0.68). EGDT was associated with greater mean (±SD) use of intensive care (5.3±7.1 vs. 4.9±7.0 days, P=0.04) and cardiovascular support (1.9±3.7 vs. 1.6±2.9 days, P=0.01) than was usual care; other outcomes did not differ significantly, although average costs were higher with EGDT. Subgroup analyses showed no benefit from EGDT for patients with worse shock (higher serum lactate level, combined hypotension and hyperlactatemia, or higher predicted risk of death) or for hospitals with a lower propensity to use vasopressors or fluids during usual resuscitation. CONCLUSIONS: In this meta-analysis of individual patient data, EGDT did not result in better outcomes than usual care and was associated with higher hospitalization costs across a broad range of patient and hospital characteristics. (Funded by the National Institute of General Medical Sciences and others; PRISM ClinicalTrials.gov number, NCT02030158.)

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Philip C Haycock1, Stephen Burgess2, Aayah Nounu1, Jie Zheng1  +194 moreInstitutions (88)
TL;DR: It is likely that longer telomeres increase risk for several cancers but reduce risk for some non-neoplastic diseases, including cardiovascular diseases, as well as single nucleotide polymorphisms (SNPs) that are strongly associated with telomere length in the general population.
Abstract: IMPORTANCE: The causal direction and magnitude of the association between telomere length and incidence of cancer and non-neoplastic diseases is uncertain owing to the susceptibility of observational studies to confounding and reverse causation. OBJECTIVE: To conduct a Mendelian randomization study, using germline genetic variants as instrumental variables, to appraise the causal relevance of telomere length for risk of cancer and non-neoplastic diseases. DATA SOURCES: Genomewide association studies (GWAS) published up to January 15, 2015. STUDY SELECTION: GWAS of noncommunicable diseases that assayed germline genetic variation and did not select cohort or control participants on the basis of preexisting diseases. Of 163 GWAS of noncommunicable diseases identified, summary data from 103 were available. DATA EXTRACTION AND SYNTHESIS: Summary association statistics for single nucleotide polymorphisms (SNPs) that are strongly associated with telomere length in the general population. MAIN OUTCOMES AND MEASURES: Odds ratios (ORs) and 95% confidence intervals (CIs) for disease per standard deviation (SD) higher telomere length due to germline genetic variation. RESULTS: Summary data were available for 35 cancers and 48 non-neoplastic diseases, corresponding to 420 081 cases (median cases, 2526 per disease) and 1 093 105 controls (median, 6789 per disease). Increased telomere length due to germline genetic variation was generally associated with increased risk for site-specific cancers. The strongest associations (ORs [95% CIs] per 1-SD change in genetically increased telomere length) were observed for glioma, 5.27 (3.15-8.81); serous low-malignant-potential ovarian cancer, 4.35 (2.39-7.94); lung adenocarcinoma, 3.19 (2.40-4.22); neuroblastoma, 2.98 (1.92-4.62); bladder cancer, 2.19 (1.32-3.66); melanoma, 1.87 (1.55-2.26); testicular cancer, 1.76 (1.02-3.04); kidney cancer, 1.55 (1.08-2.23); and endometrial cancer, 1.31 (1.07-1.61). Associations were stronger for rarer cancers and at tissue sites with lower rates of stem cell division. There was generally little evidence of association between genetically increased telomere length and risk of psychiatric, autoimmune, inflammatory, diabetic, and other non-neoplastic diseases, except for coronary heart disease (OR, 0.78 [95% CI, 0.67-0.90]), abdominal aortic aneurysm (OR, 0.63 [95% CI, 0.49-0.81]), celiac disease (OR, 0.42 [95% CI, 0.28-0.61]) and interstitial lung disease (OR, 0.09 [95% CI, 0.05-0.15]). CONCLUSIONS AND RELEVANCE: It is likely that longer telomeres increase risk for several cancers but reduce risk for some non-neoplastic diseases, including cardiovascular diseases.

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16 Oct 2017-Science
TL;DR: In this paper, ultraviolet and x-ray observations from the Nuclear Spectroscopic Telescope Array (NSTA) of the binary neutron star merger GW170817 were used to detect a high mass (≈0.03 solar masses) wind-driven outflow with moderate electron fraction.
Abstract: With the first direct detection of merging black holes in 2015, the era of gravitational wave (GW) astrophysics began. A complete picture of compact object mergers, however, requires the detection of an electromagnetic (EM) counterpart. We report ultraviolet (UV) and x-ray observations by Swift and the Nuclear Spectroscopic Telescope Array of the EM counterpart of the binary neutron star merger GW170817. The bright, rapidly fading UV emission indicates a high mass (≈0.03 solar masses) wind-driven outflow with moderate electron fraction (Ye ≈ 0.27). Combined with the x-ray limits, we favor an observer viewing angle of ≈30° away from the orbital rotation axis, which avoids both obscuration from the heaviest elements in the orbital plane and a direct view of any ultrarelativistic, highly collimated ejecta (a γ-ray burst afterglow).