output
19922026
Showing 2019 · astro-ph.HEShow all

55 papers · 2 filters

astro-ph.HE2019★ 25 cited

H.E.S.S. and Fermi-LAT observations of PSR B1259-63/LS 2883 during its 2014 and 2017 periastron passages

H. E. S. S. Collaboration, H. Abdalla, R. Adam +222

PSR B1259-63/LS 2883 is a gamma-ray binary system consisting of a pulsar in an eccentric orbit around a bright Oe stellar-type companion star that features a dense circumstellar di…

astro-ph.HE2019★ 69 cited

NICER X-ray Observations of Seven Nearby Rotation-Powered Millisecond Pulsars

S. Guillot, M. Kerr, P. S. Ray +18

NICER observed several rotation-powered millisecond pulsars to search for or confirm the presence of X-ray pulsations. When broad and sine-like, these pulsations may indicate therm…

astro-ph.HE2019★ 10 cited

Unravelling the unusually curved X-ray spectrum of RGB J0710+591 using AstroSat observations

Pranjupriya Goswami, Atreyee Sinha, Sunil Chandra +7

We report the analysis of simultaneous multi-wavelength data of the high energy peaked blazar RGB J0710+591 from the LAXPC, SXT and UVIT instruments on-board AstroSat. The wide ban…

astro-ph.HE2019★ 13 cited

Chandra Observations of High Energy X-ray Sources Discovered by INTEGRAL

John A. Tomsick, Arash Bodaghee, Sylvain Chaty +6

The International Gamma-Ray Astrophysics Laboratory (INTEGRAL) satellite has detected in excess of 1000 sources in the ~20-100 keV band during its surveys of the sky over the past…

astro-ph.HE2019★ 15 cited

Modeling spectral lags in active galactic nucleus flares in the context of Lorentz invariance violation searches

Perennes Cédric, Sol Hélène, Bolmont Julien

High-energy photons emitted by flaring active galactic nuclei (AGNs) have been used for many years to constrain modified dispersion relations in vacuum encountered in the context o…

astro-ph.HE2019★ 274 cited

A very-high-energy component deep in the Gamma-ray Burst afterglow

H. Abdalla R. Adam F. Aharonian F. Ait Benkhali E. O. Anguener M. Arakawa, C. Arcaro, C. Armand +219

Gamma-ray bursts (GRBs) are brief flashes of gamma rays, considered to be the most energetic explosive phenomena in the Universe. The emission from GRBs comprises a short (typicall…

astro-ph.HE2019★ 28 cited

H.E.S.S. detection of very-high-energy gamma-ray emission from the quasar PKS 0736+017

H. E. S. S. Collaboration, :, H. Abdalla +225

Flat-spectrum radio-quasars (FSRQs) are rarely detected at very-high-energies (VHE; E>100 GeV) due to their low-frequency-peaked SEDs. At present, only 6 FSRQs are known to emit VH…

astro-ph.HE2019★ 30 cited

Investigating the multiwavelength behaviour of the flat spectrum radio quasar CTA 102 during 2013-2017

F. D'Ammando, C. M. Raiteri, M. Villata +94

We present a multiwavelength study of the flat-spectrum radio quasar CTA 102 during 2013-2017. We use radio-to-optical data obtained by the Whole Earth Blazar Telescope, 15 GHz dat…

astro-ph.HE2019★ 76 cited

The first six months of the Advanced LIGO's and Advanced Virgo's third observing run with GRANDMA

S. Antier, S. Agayeva, V. Aivazyan +74

We present the Global Rapid Advanced Network Devoted to the Multi-messenger Addicts (GRANDMA). The network consists of 21 telescopes with both photometric and spectroscopic facilit…

astro-ph.HE2019★ 102 cited

Fast Neutrino Flavor Conversion Modes in Multidimensional Core-collapse Supernova Models: the Role of the Asymmetric Neutrino Distributions

Sajad Abbar, Huaiyu Duan, Kohsuke Sumiyoshi +2

A dense neutrino gas, such as the one anticipated in the supernova environment, can experience fast neutrino flavor conversions on scales much shorter than those expected in vacuum…

astro-ph.HE2019★ 18 cited

Constraining the cosmic ray spectrum in the vicinity of the supernova remnant W28: from sub-GeV to multi-TeV energies

V. H. M. Phan, S. Gabici, G. Morlino +4

Supernova remnants interacting with molecular clouds are ideal laboratories to study the acceleration of particles at shock waves and their transport and interactions in the surrou…

astro-ph.HE2019★ 100 cited

High angular resolution ALMA images of dust and molecules in the SN 1987A ejecta

Phil Cigan, Mikako Matsuura, Haley L. Gomez +23

We present high angular resolution (~80 mas) ALMA continuum images of the SN 1987A system, together with CO =2 1, =6 5, and SiO =5 $\!\…

astro-ph.HE2019★ 7 cited

Neutrinos from the gamma-ray source eHWC J1825-134: predictions for Km detectors

V. Niro, A. Neronov, L. Fusco +2

The eHWC J1825-134 source is located in the southern sky and has been recently detected by the HAWC observatory. It presents an hard spectral index and its gamma-ray flux extends u…

astro-ph.HE2019★ 31 cited

The 2018 outburst of BHXB H1743-322 as seen with MeerKAT

D. R. A. Williams, S. E. Motta, R. Fender +11

In recent years, the black hole candidate X-ray binary system H1743-322 has undergone outbursts and it has been observed with X-ray and radio telescopes. We present 1.3 GHz MeerKAT…

astro-ph.HE2019★ 6 cited

Polarised radiative transfer, rotation measure fluctuations and large-scale magnetic fields

Alvina Y. L. On, Jennifer Y. H. Chan, Kinwah Wu +2

Faraday rotation measure at radio wavelengths is commonly used to diagnose large-scale magnetic fields. It is argued that the length-scales on which magnetic fields vary in large-s…

astro-ph.HE2019★ 21 cited

Three-dimensional simulations of non-resonant streaming instability and particle acceleration near non-relativistic astrophysical shocks

Allard Jan van Marle, Fabien Casse, Alexandre Marcowith

We use particle-in-magnetohydrodynamics-cells to model particle acceleration and magnetic field amplification in a high Mach, parallel shock in three dimensions and compare the res…

astro-ph.HE2019★ 52 cited

Particle acceleration in relativistic turbulence: A theoretical appraisal

Camilia Demidem, Martin Lemoine, Fabien Casse

We discuss the physics of stochastic particle acceleration in relativistic magnetohydrodynamic (MHD) turbulence, combining numerical simulations of test-particle acceleration in sy…

astro-ph.HE2019★ 53 cited

Probing the Nature of Black Holes: Deep in the mHz Gravitational-Wave Sky

Vishal Baibhav, Leor Barack, Emanuele Berti +26

Black holes are unique among astrophysical sources: they are the simplest macroscopic objects in the Universe, and they are extraordinary in terms of their ability to convert energ…

astro-ph.HE2019★ 17 cited

Introduction to multi-messenger astronomy

Andrii Neronov

The new field of multi-messenger astronomy aims at the study of astronomical sources using different types of "messenger" particles: photons, neutrinos, cosmic rays and gravitation…

astro-ph.HE2019★ 68 cited

Phase transitions in neutron stars and their links to gravitational waves

Milva G. Orsaria, Germán Malfatti, Mauro Mariani +6

The recent direct observation of gravitational wave event and its signal has opened up a new window to study neutron stars and heralds a new era of Astronom…

astro-ph.HE2019★ 24 cited

Galactic diffuse gamma-ray emission at TeV energy

A. Neronov, D. V. Semikoz

Measuring the diffuse Galactic gamma-ray flux in the TeV range is difficult for ground-based gamma-ray telescopes because of the residual cosmic-ray background, which is higher tha…

astro-ph.HE2019★ 255 cited

A decade of Gamma-Ray Bursts observed by -LAT: The 2 GRB catalog

M. Axelsson, E. Bissaldi, N. Omodei +1

The Large Area Telescope (LAT) aboard the spacecraft routinely observes high-energy emission from gamma-ray bursts (GRBs). Here we present the second catalog of LAT-detecte…

astro-ph.HE2019★ 47 cited

Constraints on the emission region of 3C 279 during strong flares in 2014 and 2015 through VHE gamma-ray observations with H.E.S.S

H. E. S. S. Collaboration, H. Abdalla, R. Adam +224

The flat spectrum radio quasar 3C 279 is known to exhibit pronounced variability in the high-energy (MeVGeV) -ray band, which is continuously monitored with Fer…

astro-ph.HE2019★ 4 cited

All-Sky-ASTROGAM: The MeV Gamma-Ray Companion to Multimessenger Astronomy

V. Tatischeff, A. De Angelis, M. Tavani +33

All-Sky-ASTROGAM is a gamma-ray observatory operating in a broad energy range, 100 keV to a few hundred MeV, recently proposed as the "Fast" (F) mission of the European Space Agenc…