COSMIC cancer database
View article: COSMIC: somatic cancer genetics at high-resolution
COSMIC: somatic cancer genetics at high-resolution Open
COSMIC, the Catalogue of Somatic Mutations in Cancer (http://cancer.sanger.ac.uk) is a high-resolution resource for exploring targets and trends in the genetics of human cancer. Currently the broadest database of mutations in cancer, the i…
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The IllustrisTNG simulations: public data release Open
We present the full public release of all data from the TNG100 and TNG300 simulations of the IllustrisTNG project. IllustrisTNG is a suite of large volume, cosmological, gravo-magnetohydrodynamical simulations run with the moving-mesh code…
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First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time Open
We present a new cosmological, magnetohydrodynamical simulation for galaxy formation: TNG50, the third and final instalment of the IllustrisTNG project. TNG50 evolves 2 × 21603 dark matter particles and gas cells in a volume 50 comoving Mp…
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Inferring the star formation histories of massive quiescent galaxies with bagpipes: evidence for multiple quenching mechanisms Open
We present Bayesian Analysis of Galaxies for Physical Inference and Parameter\nEStimation, or BAGPIPES, a new Python tool which can be used to rapidly\ngenerate complex model galaxy spectra and to fit these to arbitrary\ncombinations of sp…
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Dark Energy Survey Year 1 results: Cosmological constraints from cosmic shear Open
We use 26 million galaxies from the Dark Energy Survey (DES) Year 1 shape\ncatalogs over 1321 deg$^2$ of the sky to produce the most significant\nmeasurement of cosmic shear in a galaxy survey to date. We constrain\ncosmological parameters…
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KiDS-1000 cosmology: Cosmic shear constraints and comparison between two point statistics Open
We present cosmological constraints from a cosmic shear analysis of the fourth data release of the Kilo-Degree Survey (KiDS-1000), which doubles the survey area with nine-band optical and near-infrared photometry with respect to previous K…
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Science with the Cherenkov Telescope Array Open
The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. The scientific potential of CTA is extremely broad: from understanding the role of relativis…
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Hydrogen Epoch of Reionization Array (HERA) Open
The Hydrogen Epoch of Reionization Array (HERA) is a staged experiment to measure 21 cm emission from the primordial intergalactic medium (IGM) throughout cosmic reionization (z = 6-12), and to explore earlier epochs of our Cosmic Dawn (z …
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Age-dating luminous red galaxies observed with the Southern African Large Telescope Open
We measure a value for the cosmic expansion of $H(z) = 89 \\pm 23$(stat) $\\pm$\n44(syst) km s$^{-1}$ Mpc$^{-1}$ at a redshift of $z \\simeq 0.47$ based on the\ndifferential age technique. This technique, also known as cosmic chronometers,…
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Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries Open
We explore a newly proposed channel to create binary black holes of stellar origin. This scenario applies to massive, tight binaries where mixing induced by rotation and tides transports the products of hydrogen burning throughout the stel…
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Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy\n beyond LIGO Open
This white paper describes the research and development needed over the next\ndecade to realize "Cosmic Explorer," the U.S. node of a future third-generation\ndetector network that will be capable of observing and characterizing compact\ng…
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A Comprehensive Study of Galaxies at z ∼ 9–16 Found in the Early JWST Data: Ultraviolet Luminosity Functions and Cosmic Star Formation History at the Pre-reionization Epoch Open
We conduct a comprehensive study on dropout galaxy candidates at z ∼ 9–16 using the first 90 arcmin 2 James Webb Space Telescope (JWST) Near Infrared Camera images taken by the early release observations (ERO) and early release science pro…
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Indirect dark matter signatures in the cosmic dark ages. I. Generalizing the bound on-wave dark matter annihilation from Planck results Open
Recent measurements of the cosmic microwave background (CMB) anisotropies by Planck provide a sensitive probe of dark matter annihilation during the cosmic dark ages, and specifically constrain the annihilation parameter feff=mχ. Using new…
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Testing general relativity in cosmology Open
We review recent developments and results in testing general relativity (GR) at cosmological scales. The subject has witnessed rapid growth during the last two decades with the aim of addressing the question of cosmic acceleration and the …
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Cosmic microwave background limits on accreting primordial black holes Open
Interest in the idea that primordial black holes (PBHs) might comprise some or all of the dark matter has recently been rekindled following LIGO's first direct detection of a binary-black-hole merger. Here we revisit the effect of accretin…
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Evidence for neutrino emission from the nearby active galaxy NGC 1068 Open
A supermassive black hole, obscured by cosmic dust, powers the nearby active galaxy NGC 1068. Neutrinos, which rarely interact with matter, could provide information on the galaxy’s active core. We searched for neutrino emission from astro…
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The cosmic baryon cycle and galaxy mass assembly in the FIRE simulations Open
We use cosmological simulations from the FIRE (Feedback In Realistic Environments) project to study the baryon cycle and galaxy mass assembly for central galaxies in the halo mass range Mhalo ∼ 10^(10)–10^(13) M_⊙. By tracing cosmic inflow…
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Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration Open
This work, together with its companion paper, Secco, Samuroff et al. [Phys. Rev. D 105, 023515 (2022)PRVDAQ2470-001010.1103/PhysRevD.105.023515], present the Dark Energy Survey Year 3 cosmic-shear measurements and cosmological constraints …
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Observation of a large-scale anisotropy in the arrival directions of cosmic rays above 8 × 10 <sup>18</sup> eV Open
High-energy particles are extragalactic Cosmic rays are high-energy particles arriving from space; some have energies far beyond those that human-made particle accelerators can achieve. The sources of higher-energy cosmic rays remain under…
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<i>Euclid</i> preparation Open
Aims. The Euclid space telescope will measure the shapes and redshifts of galaxies to reconstruct the expansion history of the Universe and the growth of cosmic structures. The estimation of the expected performance of the experiment, in t…
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The VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release Open
We present the VLA-COSMOS 3 GHz Large Project based on 384 hours of\nobservations with the Karl G. Jansky Very Large Array (VLA) at 3 GHz (10 cm)\ntoward the two square degree Cosmic Evolution Survey (COSMOS) field. The final\nmosaic reach…
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Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty Open
This work and its companion paper, Amon et al. [Phys. Rev. D 105, 023514 (2022)], present cosmic shear measurements and cosmological constraints from over 100 million source galaxies in the Dark Energy Survey (DES) Year 3 data. We constrai…
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Fundamental physics with the Square Kilometre Array Open
The Square Kilometre Array (SKA) is a planned large radio interferometer designed to operate over a wide range of frequencies, and with an order of magnitude greater sensitivity and survey speed than any current radio telescope. The SKA wi…
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Hidden Cosmic-Ray Accelerators as an Origin of TeV-PeV Cosmic Neutrinos Open
The latest IceCube data suggest that the all-flavor cosmic neutrino flux may be as large as 10^{-7} GeV cm^{-2} s^{-1} sr^{-1} around 30 TeV. We show that, if sources of the TeV-PeV neutrinos are transparent to γ rays with respect to two-p…
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Precision Measurement of the Boron to Carbon Flux Ratio in Cosmic Rays from 1.9 GV to 2.6 TV with the Alpha Magnetic Spectrometer on the International Space Station Open
Knowledge of the rigidity dependence of the boron to carbon flux ratio (B/C) is important in understanding the propagation of cosmic rays. The precise measurement of the B/C ratio from 1.9 GV to 2.6 TV, based on 2.3 million boron and 8.3 m…
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The Romulus cosmological simulations: a physical approach to the formation, dynamics and accretion models of SMBHs Open
We present a novel implementation of supermassive black hole (SMBH)\nformation, dynamics, and accretion in the massively parallel tree+SPH code,\nChaNGa. This approach improves the modeling of SMBHs in fully cosmological\nsimulations, allo…
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Tracing the cosmic web Open
The cosmic web is one of the most striking features of the distribution of\ngalaxies and dark matter on the largest scales in the Universe. It is composed\nof dense regions packed full of galaxies, long filamentary bridges, flattened\nshee…
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The SCUBA-2 Cosmology Legacy Survey: 850 μm maps, catalogues and number counts Open
We present a catalogue of ∼3000 submillimetre sources detected (≥3.5σ) at 850 μm over ∼5 deg2 surveyed as part of the James Clerk Maxwell Telescope (JCMT) SCUBA-2 Cosmology Legacy Survey (S2CLS). This is the largest survey of its kind at 8…
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Probing cosmic inflation with the<i>LiteBIRD</i>cosmic microwave background polarization survey Open
LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for primordial cosmology and fundamental physics. The Japan Aerospace Exploration Agency…
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A Multimessenger Picture of the Flaring Blazar TXS 0506+056: Implications for High-energy Neutrino Emission and Cosmic-Ray Acceleration Open
Detection of the IceCube-170922A neutrino coincident with the flaring blazar TXS 0506+056, the first and only ∼3 σ high-energy neutrino source association to date, offers a potential breakthrough in our understanding of high-energy cosmic …