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20002026
most citedSpectroscopic identification of r-process nucleosynthesis in a double neutron star merger

1k citations · 14.2k across the 235 of their papers we have counts for

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Showing 2022Show all

9 papers · 1 filter

astro-ph.HE2022★ 8 cited

Finding high-redshift gamma-ray bursts in tandem near-infrared and optical surveys

S. Campana, G. Ghirlanda, R. Salvaterra +8

The race for the most distant object in the Universe has been played by long-duration gamma-ray bursts (GRBs), star-forming galaxies and quasars. GRBs took a temporary lead with th…

astro-ph.HE2022★ 1 cited

The Cosmic History of Long Gamma Ray Bursts

G. Ghirlanda, R. Salvaterra

The cosmic formation rate of long Gamma Ray Bursts (LGRBs) encodes the evolution, across cosmic times, of their progenitors' properties and of their environment. The LGRB formation…

astro-ph.HE2022★ 4 cited

The Structure of Gamma Ray Burst Jets

Om Sharan Salafia, Giancarlo Ghirlanda

Due to relativistic bulk motion, the structure and orientation of gamma-ray burst jets have a fundamental role in determining how they appear. The recent discovery of the GW170817…

astro-ph.HE2022★ 11 cited

VLBI observations of GRB 201015A, a relatively faint GRB with a hint of Very High Energy gamma-ray emission

S. Giarratana, L. Rhodes, B. Marcote +14

GRB 201015A is a long-duration Gamma-Ray Burst (GRB) which was detected at very high energies (> 100 GeV) using the MAGIC telescopes. If confirmed, this would be the fifth and leas…

astro-ph.HE2022★ 72 cited

GeV emission from a compact binary merger

Alessio Mei, Biswajit Banerjee, Gor Oganesyan +9

An energetic -ray burst (GRB), GRB 211211A, was observed on 2021 December 11 by the Neil Gehrels Swift Observatory. Despite its long duration, typically associated with burs…

astro-ph.HE2022★ 70 cited

Multi-messenger observations of binary neutron star mergers in the O4 run

A. Colombo, O. S. Salafia, F. Gabrielli +4

We present realistic expectations for the number and properties of neutron star binary mergers to be detected as multi-messenger sources during the upcoming fourth observing run (O…