output
19932026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2018 · astro-ph.HEShow all

41 papers · 2 filters

astro-ph.HE2018★ 72 cited

Observatory science with eXTP

Jean J. M. in 't Zand, Enrico Bozzo, Jinlu Qu +181

In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring s…

astro-ph.HE2018★ 135 cited

Dense matter with eXTP

Anna L. Watts, Wenfei Yu, Juri Poutanen +73

In this White Paper we present the potential of the Enhanced X-ray Timing and Polarimetry (eXTP) mission for determining the nature of dense matter; neutron star cores host an extr…

astro-ph.HE2018★ 44 cited

Photoionized emission and absorption features in the high-resolution X-ray spectra of NGC 3783

Junjie Mao, M. Mehdipour, J. S. Kaastra +14

Our Swift monitoring program triggered two joint XMM-Newton, NuSTAR and HST observations on 11 and 21 December 2016 targeting NGC 3783, as its soft X-ray continuum was heavily obsc…

astro-ph.HE2018★ 19 cited

Study of the X-ray pulsar IGR J19294+1816 with NuSTAR: detection of cyclotron line and transition to accretion from the cold disc

Sergey S. Tsygankov, Victor Doroshenko, Alexander A. Mushtukov +2

In the work we present the results of two deep broad-band observations of the poorly studied X-ray pulsar IGR J19294+1816 obtained with the NuSTAR observatory. The source was obser…

astro-ph.HE2018★ 56 cited

Radio observations of the merging galaxy cluster Abell 520

D. N. Hoang, T. W. Shimwell, R. J. van Weeren +13

We examine the possible acceleration mechanisms of the relativistic particles responsible for the extended radio emission in Abell 520. We used new LOFAR 145 MHz, archival GMRT 323…

astro-ph.HE2018★ 22 cited

Characterizing the radio emission from the binary galaxy cluster merger Abell 2146

D. N. Hoang, T. W. Shimwell, R. J. van Weeren +8

Collisions of galaxy clusters generate shocks and turbulence in the intra-cluster medium (ICM). The presence of relativistic particles and magnetic fields is inferred through the d…

astro-ph.HE2018★ 18 cited

Blazars in the LOFAR Two-Metre Sky Survey First Data Release

S. Mooney, J. Quinn, J. R. Callingham +13

Historically, the blazar population has been poorly understood at low frequencies because survey sensitivity and angular resolution limitations have made it difficult to identify m…

astro-ph.HE2018★ 68 cited

The intergalactic magnetic field probed by a giant radio galaxy

S. P. O'Sullivan, J. Machalski, C. L. Van Eck +27

Cosmological simulations predict that an intergalactic magnetic field (IGMF) pervades the large scale structure (LSS) of the Universe. Measuring the IGMF is important to determine…

astro-ph.HE2018★ 13 cited

X-ray spectroscopy of galaxy clusters: beyond the CIE modeling

Liyi Gu, Irina Zhuravleva, Eugene Churazov +3

X-ray spectra of galaxy clusters are dominated by the thermal emission from the hot intracluster medium. In some cases, besides the thermal component, spectral models require addit…

astro-ph.HE2018★ 3 cited

The Signature of a Windy Radio Supernova Progenitor in a Binary System

Almog Yalinewich, Simon Portegies Zwart

Type II supernova progenitors are expected to emit copious amounts of mass in a dense stellar wind prior to the explosion. When the progenitor is a member of a binary, the orbital…

astro-ph.HE2018★ 195 cited

The First Swift Intensive AGN Accretion Disk Reverberation Mapping Survey

R. Edelson, J. Gelbord, E. Cackett +32

Swift intensive accretion disk reverberation mapping of four AGN yielded light curves sampled 200-350 times in 0.3-10 keV X-ray and six UV/optical bands. Uniform reduction an…

astro-ph.HE2018★ 69 cited

Timing properties of ULX pulsars: optically thick envelopes and outflows

Alexander A. Mushtukov, Adam Ingram, Matthew Middleton +2

It has recently been discovered that a fraction of ultra-luminous X-ray sources (ULXs) exhibit X-ray pulsations, and are therefore powered by super-Eddington accretion onto magneti…

astro-ph.HE2018★ 82 cited

Enrichment of the hot intracluster medium: observations

F. Mernier, V. Biffi, H. Yamaguchi +7

Four decades ago, the firm detection of an Fe-K emission feature in the X-ray spectrum of the Perseus cluster revealed the presence of iron in its hot intracluster medium (ICM). Wi…

astro-ph.HE2018★ 17 cited

A low-frequency view of mixed-morphology supernova remnant VRO 42.05.01, and its neighbourhood

M. Arias, J. Vink, M. Iacobelli +7

Mixed-morphology supernova remnants (MM SNRs) are a mysterious class of objects that display thermal X-ray emission within their radio shell. They are an older class of SNRs, and a…

astro-ph.HE2018★ 59 cited

Dramatic spectral transition of X-ray pulsar GX 304-1 in low luminous state

Sergey S. Tsygankov, Alicia Rouco Escorial, Valery Suleimanov +5

We report on the discovery of a dramatic change in the energy spectrum of the X-ray pulsar GX 304-1 appearing at low luminosity. Particularly, we found that the cutoff power-law sp…

astro-ph.HE2018★ 138 cited

Sensitivity of the KM3NeT/ARCA neutrino telescope to point-like neutrino sources

The KM3NeT Collaboration, S. Aiello, S. E. Akrame +219

KM3NeT will be a network of deep-sea neutrino telescopes in the Mediterranean Sea. The KM3NeT/ARCA detector, to be installed at the Capo Passero site (Italy), is optimised for the…

astro-ph.HE2018★ 39 cited

Detection of polarized gamma-ray emission from the Crab nebula with Hitomi Soft Gamma-ray Detector

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +191

We present the results from the Hitomi Soft Gamma-ray Detector (SGD) observation of the Crab nebula. The main part of SGD is a Compton camera, which in addition to being a spectrom…

astro-ph.HE2018★ 21 cited

Nitrogen abundance in the X-ray halos of clusters and groups of galaxies

Junjie Mao, J. de Plaa, J. S. Kaastra +6

Chemical abundances in the X-ray halos (also known as the intracluster medium, ICM) of clusters and groups of galaxies can be measured via prominent emission line features in their…

astro-ph.HE2018★ 15 cited

An ultra-fast inflow in the luminous Seyfert PG1211+143

Ken Pounds, Chris Nixon, Andrew Lobban +1

Blueshifted absorption lines in the X-ray spectra of AGN show that ultra-fast outflows with typical velocities are a common feature of these luminous objects. Such po…

astro-ph.HE2018★ 32 cited

X-ray Structure between the Innermost Disk and Optical Broad Line Region in NGC 4151

J. M. Miller, E. Cackett, A. Zoghbi +9

We present an analysis of the narrow Fe K-alpha line in Chandra/HETGS observations of the Seyfert AGN, NGC 4151. The sensitivity and resolution afforded by the gratings reveal asym…

astro-ph.HE2018★ 19 cited

Circumbinary discs around merging stellar-mass black holes

Rebecca G. Martin, Chris Nixon, Fu-Guo Xie +1

A circumbinary disc around a pair of merging stellar-mass black holes may be shocked and heated during the recoil of the merged hole, causing a near-simultaneous electromagnetic co…

astro-ph.HE2018★ 92 cited

Joint constraints on Galactic diffuse neutrino emission from ANTARES and IceCube

A. Albert, M. André, M. Anghinolfi +454

The existence of diffuse Galactic neutrino production is expected from cosmic ray interactions with Galactic gas and radiation fields. Thus, neutrinos are a unique messenger offeri…

astro-ph.HE2018★ 395 cited

Compact radio emission indicates a structured jet was produced by a binary neutron star merger

G. Ghirlanda, O. S. Salafia, Z. Paragi +33

The binary neutron star merger event GW170817 was detected through both electromagnetic radiation and gravitational waves. Its afterglow emission may have been produced by either a…

astro-ph.HE2018★ 20 cited

The cosmic ray shadow of the Moon observed with the ANTARES neutrino telescope

A. Albert, M. André, M. Anghinolfi +124

One of the main objectives of the ANTARES telescope is the search for point-like neutrino sources. Both the pointing accuracy and the angular resolution of the detector are importa…