activity
20052021
most citedA bright gamma-ray flare interpreted as a giant magnetar flare in NGC 253

101 citations · 123 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2021101 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

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.SR201711 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.HE2013

GRB 080407: an ultra-long burst discovered by the IPN

V. Pal'shin, K. Hurley, J. Goldsten +25

We present observations of the extremely long GRB 080704 obtained with the instruments of the Interplanetary Network (IPN). The observations reveal two distinct emission episodes,…

astro-ph.HE201311 cited

Extremely long hard bursts observed by Konus-Wind

V. Pal'shin, R. Aptekar, D. Frederiks +18

We report the observations of the prompt emission of the extremely long hard burst, GRB 060814B, discovered by Konus-Wind and localized by the IPN. The observations reveal a smooth…

astro-ph2005

An exceptionally bright flare from SGR1806-20 and the origins of short-duration gamma-ray bursts

K. Hurley, S. E. Boggs, D. M. Smith +17

Soft-gamma-ray repeaters (SGRs) are galactic X-ray stars that emit numerous short-duration (about 0.1 s) bursts of hard X-rays during sporadic active periods. They are thought to b…