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19982021
most citedSpectroscopic identification of r-process nucleosynthesis in a double neutron star merger

1k citations · 5.7k across the 46 of their papers we have counts for

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Showing 2020Show all

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astro-ph.HE2020

10.4m GTC observations of the nearby VHE-detected GRB 190829A/SN 2019oyw

Y. -D. Hu, A. J. Castro-Tirado, A. Kumar +15

Aims. GRB 190829A (z = 0.0785), detected by Fermi and Swift with two emission episodes separated by a quiescent gap of ~40 s, was also observed by the H.E.S.S. telescopes at Very-H…

astro-ph.HE2020

INTEGRAL view of AGN

Angela Malizia, Sergey Sazonov, Loredana Bassani +5

AGN are among the most energetic phenomena in the Universe and in the last two decades INTEGRAL's contribution in their study has had a significant impact. Thanks to the INTEGRAL e…

astro-ph.HE2020

Mergers of binary neutron star systems: a multi-messenger revolution

Elena Pian

On 17 August 2017, less than two years after the direct detection of gravitational radiation from the merger of two ~30 Msun black holes, a binary neutron star merger was identifie…

astro-ph.HE20209 cited

PTF11rka: an interacting supernova at the crossroads of stripped-envelope and H-poor super-luminous stellar core collapses

Elena Pian, Paolo A. Mazzali, Takashi J. Moriya +17

The hydrogen-poor supernova PTF11rka (z = 0.0744), reported by the Palomar Transient Factory, was observed with various telescopes starting a few days after the estimated explosion…

astro-ph.HE2020

Kilonova Luminosity Function Constraints based on Zwicky Transient Facility Searches for 13 Neutron Star Mergers

Mansi M. Kasliwal, Shreya Anand, Tomas Ahumada +100

We present a systematic search for optical counterparts to 13 gravitational wave (GW) triggers involving at least one neutron star during LIGO/Virgo's third observing run. We searc…

astro-ph.HE202036 cited

A Supernova Candidate at z=0.092 in XMM-Newton Archival Data

G. Novara, P. Esposito, A. Tiengo +14

During a search for X-ray transients in the XMM-Newton archive within the EXTraS project, we discovered a new X-ray source that is detected only during a ~5 min interval of a ~21 h…