output
19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2017 · astro-ph.HEShow all

30 papers · 2 filters

astro-ph.HE2017★ 41 cited

Studying the Ultraviolet Spectrum of the First Spectroscopically Confirmed Supernova at redshift two

M. Smith, M. Sullivan, R. C. Nichol +87

We present observations of DES16C2nm, the first spectroscopically confirmed hydrogen-free superluminous supernova (SLSN-I) at redshift z~2. DES16C2nm was discovered by the Dark Ene…

astro-ph.HE2017★ 72 cited

Evidence for Dynamically Driven Formation of the GW170817 Neutron Star Binary in NGC 4993

A. Palmese, W. Hartley, F. Tarsitano +89

We present a study of NGC 4993, the host galaxy of the GW170817 gravitational wave event, the GRB170817A short gamma-ray burst (sGRB) and the AT2017gfo kilonova. We use Dark Energy…

astro-ph.HE2017★ 84 cited

Ultra-High Energy Cosmic Rays and Neutrinos from Tidal Disruptions by Massive Black Holes

Claire Guépin, Kumiko Kotera, Enrico Barausse +2

Tidal disruptions are extremely powerful phenomena that have been designated as candidate sources of ultra-high-energy cosmic rays. The disruption of a star by a black hole can nat…

astro-ph.HE2017★ 42 cited

Retainment of r-process material in dwarf galaxies

Paz Beniamini, Irina Dvorkin, Joe Silk

The synthesis of -process elements is known to involve extremely energetic explosions. At the same time, recent observations find significant -process enrichment even in extr…

astro-ph.HE2017★ 27 cited

Fermionic Light Dark Matter particles and the New Physics of Neutron Stars

M. Cermeño, M. Ángeles Pérez-García, Joseph Silk

Dark Matter constitutes most of the matter in the presently accepted cosmological model for our Universe. The extreme conditions of ordinary baryonic matter, namely high density an…

astro-ph.HE2017★ 888 cited

A kilonova as the electromagnetic counterpart to a gravitational-wave source

S. J. Smartt, T. -W. Chen, A. Jerkstrand +118

Gravitational waves were discovered with the detection of binary black hole mergers and they should also be detectable from lower mass neutron star mergers. These are predicted to…

astro-ph.HE2017★ 1k cited

The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

P. S. Cowperthwaite, E. Berger, V. A. Villar +141

We present UV, optical, and NIR photometry of the first electromagnetic counterpart to a gravitational wave source from Advanced LIGO/Virgo, the binary neutron star merger GW170817…

astro-ph.HE2017★ 584 cited

The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart

M. Soares-Santos, D. E. Holz, J. Annis +142

We present the Dark Energy Camera (DECam) discovery of the optical counterpart of the first binary neutron star merger detected through gravitational wave emission, GW170817. Our o…

astro-ph.HE2017★ 12 cited

Relativistic magnetohydrodynamical simulations of the resonant corrugation of a fast shock front

Camilia Demidem, Martin Lemoine, Fabien Casse

The generation of turbulence at magnetized shocks and its subsequent interaction with the latter is a key question of plasma- and high-energy astrophysics. This paper presents two-…

astro-ph.HE2017★ 26 cited

Exploring stellar evolution with gravitational-wave observations

Irina Dvorkin, Jean-Philippe Uzan, Elisabeth Vangioni +1

Recent detections of gravitational waves from merging binary black holes opened new possibilities to study the evolution of massive stars and black hole formation. In particular, s…

astro-ph.HE2017★ 4 cited

Dark matter line searches towards dwarf galaxies with H.E.S.S

Louise Oakes, Aion Viana, Emmanuel Moulin +7

High energy -rays are powerful probes in the search for annihilations of dark matter (DM) par- ticles in dense environments. In several DM particle models their annihilation pro…

astro-ph.HE2017★ 27 cited

Search for gamma-ray emission from super-luminous supernovae with the Fermi-LAT

Nicolas Renault-Tinacci, Kumiko Kotera, Andrii Neronov +1

We present the first individual and stacking systematic search for -ray emission in the GeV band with the {\it Fermi} Large Area Telescope (LAT), in the directions of 45 super-l…

astro-ph.HE2017★ 16 cited

LSQ14efd: observations of the cooling of a shock break-out event in a type Ic Supernova

C. Barbarino, M. T. Botticella, M. Dall'Ora +29

We present the photometric and spectroscopic evolution of the type Ic supernova LSQ14efd, discovered by the La Silla QUEST survey and followed by PESSTO. LSQ14efd was discovered fe…

astro-ph.HE2017★ 43 cited

The host galaxy of the short GRB111117A at : impact on the short GRB redshift distribution and progenitor channels

J. Selsing, T. Krühler, D. Malesani +26

It is notoriously difficult to localize short -ray bursts (sGRBs) and their hosts to measure their redshifts. These measurements, however, are critical to constrain the nature o…

astro-ph.HE2017★ 7 cited

Multi-epoch intra-night optical monitoring of 8 radio-quiet BL Lac candidates

P. Kumar, Gopal-Krishna, C. S. Stalin +3

For a new sample of 8 weak-line-quasars (WLQs) we report a sensitive search in 20 intranight monitoring sessions, for blazar-like optical flux variations on hour-like and longer ti…

astro-ph.HE2017★ 364 cited

The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes

K. Belczynski, J. Klencki, C. E. Fields +31

All ten LIGO/Virgo binary black hole (BH-BH) coalescences reported from the O1/O2 runs have near zero effective spins. There are only three potential explanations of this fact. If…

astro-ph.HE2017★ 41 cited

Towards understanding the physics of collisionless relativistic shocks

Guy Pelletier, Andrei Bykov, Don Ellison +1

Relativistic astrophysical collisionless shocks represent outstanding dissipation agents of the huge power of relativistic outflows produced by accreting black holes, core collapse…

astro-ph.HE2017★ 38 cited

What can we learn from "internal plateaus"? The peculiar afterglow of GRB 070110

Paz Beniamini, Robert Mochkovitch

Context: The origin of GRBs' prompt emission is highly debated. Proposed scenarios involve dissipation processes above or below the photosphere of an ultra-relativistic outflow. Ai…

astro-ph.HE2017★ 20 cited

Time evolution of the spectral break in the high-energy extra component of GRB 090926A

M. Yassine, F. Piron, R. Mochkovitch +1

We report on a new time-resolved analysis of the GRB 090926A broad-band spectrum during its prompt phase, and on its interpretation in the framework of prompt emission models. We c…

astro-ph.HE2017★ 73 cited

The origin of the Ultraluminous X-ray Sources

Grzegorz Wiktorowicz, Małgorzata Sobolewska, Jean-Pierre Lasota +1

Recently, several ultraluminous X-ray (ULX) sources were shown to host a neutron star (NS) accretor. We perform a suite of evolutionary calculations which show that, in fact, NSs a…

astro-ph.HE2017★ 66 cited

Prompt Gamma Ray Burst emission from gradual magnetic dissipation

Paz Beniamini, Dimitrios Giannios

We considered a model for the prompt phase of Gamma-Ray Burst (GRB) emission arising from a magnetized jet undergoing gradual energy dissipation due to magnetic reconnection. The d…

astro-ph.HE2017★ 7 cited

X-ray Insights into the Nature of Quasars with Redshifted Broad Absorption Lines

Ning-Xiao Zhang, W. N. Brandt, N. S. Ahmed +8

We present observations of seven broad absorption line (BAL) quasars at -2.516 with redshifted BAL troughs (RSBALs). Five of our seven targets were detected by $…

astro-ph.HE2017★ 80 cited

The fine line between total and partial tidal disruption events

Deborah Mainetti, Alessandro Lupi, Sergio Campana +4

Flares from tidal disruption events are unique tracers of quiescent black holes at the centre of galaxies. The appearance of these flares is very sensitive to whether the star is t…

astro-ph.HE2017★ 3 cited

The elusive synchrotron precursor of collisionless shocks

Ruben Zakine, Martin Lemoine

Most of the plasma microphysics which shapes the acceleration process of particles at collisionless shock waves takes place in the cosmic-ray precursor, through the interaction of…