output
19932026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

Showing 2019 · astro-ph.HEShow all

43 papers · 2 filters

astro-ph.HE2019★ 10 cited

A New Microquasar Candidate in M83

Roberto Soria, William P. Blair, Knox S. Long +2

Microquasars are neutron star or black hole X-ray binaries with jets. These jets can create shock-ionized bubbles of hot plasma that can masquerade as peculiar supernova remnants (…

astro-ph.HE2019★ 4 cited

GRB 190114C in the nuclear region of an interacting galaxy -- A detailed host analysis using ALMA, HST and VLT

A. de Ugarte Postigo, C. C. Thöne, S. Martın +28

GRB 190114C is the first GRB for which the detection of very-high energy emission up to the TeV range has been reported. It is still unclear whether environmental properties might…

astro-ph.HE2019★ 28 cited

NuSTAR Uncovers an Extremely Local Compton-thick AGN in NGC 4968

Stephanie M. LaMassa, Tahir Yaqoob, Peter G. Boorman +5

We present the analysis of Chandra and NuSTAR spectra of NGC 4968, a local (D44 Mpc) 12m-selected Seyfert 2 galaxy, enshrouded within Compton-thick layers of obscuring gas…

astro-ph.HE2019★ 28 cited

Incoherent fast variability of X-ray obscurers. The case of NGC 3783

B. De Marco, T. P. Adhikari, G. Ponti +22

Context. Obscuration events caused by outflowing clumps or streams of high column density, low ionisation gas, heavily absorbing the X-ray continuum, have been witnessed in a numbe…

astro-ph.HE2019★ 27 cited

The late-time radio behavior of GRB afterglows: testing the standard model

Tuomas Kangas, Andrew Fruchter

We examine a sample of 21 gamma-ray burst (GRB) afterglow light curves at radio frequencies, and compare them to the X-ray and/or optical properties of the afterglows and to the pr…

astro-ph.HE2019★ 19 cited

GRB 180620A: Evidence for late-time energy injection

Rosa L. Becerra, Fabio De Colle, Alan M. Watson +11

The early optical emission of gamma-ray bursts gives an opportunity to understand the central engine and first stages of these events. About 30\% of GRBs present flares whose origi…