activity
20052026
most citedVery high energy particle acceleration powered by the jets of the microquasar SS 433

153 citations · 523 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2026

High-redshift GRB 140304A at z = 5.282 with flaring activity: A multi-wavelength study

Shashi. B. Pandey, Amit. K. Ror, A. J. Castro-Tirado +48

Context. This article presents a detailed multi-wavelength analysis of GRB 140304A at z = 5.282, having uncommon late-time flaring features. The aim is to study GRB 140304A and oth…

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.HE2020★ 13 cited

Modelling the prompt optical emission of GRB 180325A: the evolution of a spike from the optical to gamma-rays

Rosa L. Becerra, Fabio De Colle, Jorge Cantó +20

The transition from prompt to the afterglow emission is one of the most exciting and least understood phases in gamma-ray bursts (GRBs). Correlations among optical, X-ray and gamma…

astro-ph.HE2020★ 3 cited

Constraints on the Emission of Gamma Rays from M31 with HAWC

HAWC Collaboration, A. Albert, R. Alfaro +82

Cosmic rays, along with stellar radiation and magnetic fields, are known to make up a significant fraction of the energy density of galaxies such as the Milky Way. When cosmic rays…

astro-ph.HE2019★ 12 cited

HAWC Contributions to the 36th International Cosmic Ray Conference (ICRC2019)

A. U. Abeysekara, A. Albert, R. Alfaro +127

List of proceedings from the HAWC Collaboration presented at the 36th International Cosmic Ray Conference, 24 July - 1 August 2019, Madison, Wisconsin, USA.

astro-ph.HE2019★ 28 cited

Reverse Shock Emission Revealed in Early Photometry in the Candidate Short GRB 180418A

Rosa L. Becerra, Simone Dichiara, Alan M. Watson +14

We present observations of the possible short GRB 180418A in -rays, X-rays, and in the optical. Early optical photometry with the TAROT and RATIR instruments show a bright peak…