activity
19972024
most citedInverse Compton X-ray Emission from Supernovae with Compact Progenitors: Application to SN2011fe

122 citations · 709 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.HE2024

Investigating Polarization characteristics of GRB200503A and GRB201009A

Divita Saraogi, Suman Bala, Jitendra Joshi +18

We present results of a comprehensive analysis of the polarization characteristics of GRB 200503A and GRB 201009A observed with the Cadmium Zinc Telluride Imager (CZTI) on board As…

astro-ph.HE2021★ 101 cited

A bright gamma-ray flare interpreted as a giant magnetar flare in NGC 253

D. Svinkin, D. Frederiks, K. Hurley +33

Magnetars are young, highly magnetized neutron stars that produce extremely rare giant flares of gamma-rays, the most luminous astrophysical phenomena in our Galaxy. The detection…

astro-ph.SR2018★ 27 cited

Radio, Hard X-Ray, and Gamma-Ray Emissions Associated with a Far-Side Solar Event

V. V. Grechnev, V. I. Kiselev, L. K. Kashapova +9

The SOL2014-09-01 far-side solar eruptive event produced hard electromagnetic and radio emissions observed with detectors at near-Earth vantage points. Especially challenging was a…

astro-ph.SR2018★ 4 cited

New estimation of non-thermal electron energetics in the giant solar flare on 28 October 2003 based on Mars Odyssey observations

B. A. Nizamov, I. V. Zimovets, D. V. Golovin +5

A new estimation of the total number and energy of the non-thermal electrons produced in the giant () solar flare on 2003 October 28 is presented based on the analysis…

astro-ph.SR2017★ 11 cited

Catalog of Hard X-ray Solar Flares Detected with Mars Odyssey/HEND from the Mars Orbit in 2001-2016

M. A. Livshits, I. V. Zimovets, D. V. Golovin +7

The study of nonstationary processes in the Sun is of great interest, and lately, multiwavelength observations and registration of magnetic fields are carried out by means of both…

astro-ph.HE2014★ 53 cited

A Missing-Link in the Supernova-GRB Connection: The Case of SN 2012ap

Sayan Chakraborti, Alicia Soderberg, Laura Chomiuk +50

Gamma Ray Bursts (GRBs) are characterized by ultra-relativistic outflows, while supernovae are generally characterized by non-relativistic ejecta. GRB afterglows decelerate rapidly…