activity
20142023
most citedGRB 221009A: Discovery of an Exceptionally Rare Nearby and Energetic Gamma-Ray Burst

112 citations · 258 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2023

An Explanation of GRB Fermi-LAT Flares and High-Energy Photons in Stratified Afterglows

Nissim Fraija, Boris Betancourt Kamenetskaia, Antonio Galván-Gámez +6

The second {\itshape Fermi}/LAT gamma-ray burst (GRB) catalog (2FLGC) spanning the first decade of operations by the LAT collaboration was recently released. The closure relations…

astro-ph.HE2023

Machine-Learning Enhanced Photometric Analysis of the Extremely Bright GRB 210822A

Camila Angulo-Valdez, Rosa L. Becerra, Margarita Pereyra +16

We present analytical and numerical models of the bright long GRB 210822A at . The intrinsic extreme brightness exhibited in the optical, which is very similar to other br…

astro-ph.HE2023

Understanding the Nature of the Optical Emission in Gamma-Ray Bursts: Analysis from TAROT, COATLI, and RATIR Observations

R. L. Becerra, A. Klotz, J. L. Atteia +12

We collected the optical light curve data of 227 gamma-ray bursts (GRBs) observed with the TAROT, COATLI, and RATIR telescopes. These consist of 133 detections and 94 upper limits.…

astro-ph.HE20239 cited

A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst

Yu-Han Yang, Eleonora Troja, Brendan O'Connor +24

Kilonovae are a rare class of astrophysical transients powered by the radioactive decay of nuclei heavier than iron, synthesized in the merger of two compact objects. Over the firs…

astro-ph.HE202316 cited

Heavy element nucleosynthesis associated with a gamma-ray burst

James H. Gillanders, Eleonora Troja, Chris L. Fryer +9

Kilonovae are a novel class of astrophysical transients, and the only observationally-confirmed site of rapid neutron capture nucleosynthesis (the r-process) in the Universe. To da…

astro-ph.HE202318 cited

Deciphering the unusual stellar progenitor of GRB 210704A

R. L. Becerra, E. Troja, A. M. Watson +16

GRB~210704A is a burst of intermediate duration (~s) followed by a fading afterglow and an optical excess that peaked about 7 days after the explosion. Its propert…