activity
20022024
most citedAn exceptionally bright flare from SGR1806-20 and the origins of short-duration gamma-ray bursts

598 citations · 1.2k across the 18 of their papers we have counts for

collaborators

18 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★ 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…

astro-ph.HE2013★ 36 cited

The ultraluminous GRB 110918A

D. D. Frederiks, K. Hurley, D. S. Svinkin +29

GRB 110918A is the brightest long GRB detected by Konus-WIND during its 19 years of continuous observations and the most luminous GRB ever observed since the beginning of the cosmo…

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.HE2013★ 11 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-ph.HE2013★ 2 cited

IPN localizations of Konus short gamma-ray bursts

V. D. Pal'shin, K. Hurley, D. S. Svinkin +71

Between the launch of the \textit{GGS Wind} spacecraft in 1994 November and the end of 2010, the Konus-\textit{Wind} experiment detected 296 short-duration gamma-ray bursts (includ…

astro-ph.HE2013★ 59 cited

The Interplanetary Network Supplement to the Fermi GBM Catalog of Cosmic Gamma-Ray Bursts

K. Hurley, V. D. Pal'shin, R. L. Aptekar +37

We present Interplanetary Network (IPN) data for the gamma-ray bursts in the first Fermi Gamma-Ray Burst Monitor (GBM) catalog. Of the 491 bursts in that catalog, covering 2008 Jul…

astro-ph.HE2012★ 122 cited

Inverse Compton X-ray Emission from Supernovae with Compact Progenitors: Application to SN2011fe

R. Margutti, A. M. Soderberg, L. Chomiuk +35

We present a generalized analytic formalism for the inverse Compton X-ray emission from hydrogen-poor supernovae and apply this framework to SN2011fe using Swift-XRT, UVOT and Chan…

astro-ph.HE2011★ 1 cited

The Interplanetary Network Supplement to the Fermi GBM Catalog - An AO-2 and AO-3 Guest Investigator Project

K. Hurley, M. Briggs, V. Connaughton +37

In the first two years of operation of the Fermi GBM, the 9-spacecraft Interplanetary Network (IPN) detected 158 GBM bursts with one or two distant spacecraft, and triangulated the…

astro-ph.HE2010★ 9 cited

The Interplanetary Network Supplement to the BeppoSAX Gamma-Ray Burst Catalogs

K. Hurley, C. Guidorzi, F. Frontera +31

Between 1996 July and 2002 April, one or more spacecraft of the interplanetary network detected 787 cosmic gamma-ray bursts that were also detected by the Gamma-Ray Burst Monitor a…

astro-ph.HE2009

Integrating the Fermi Gamma-Ray Burst Monitor into the 3rd Interplanetary Network

K. Hurley, M. Briggs, V. Connaughton +35

We are integrating the Fermi Gamma-Ray Burst Monitor (GBM) into the Interplanetary Network (IPN) of Gamma-Ray Burst (GRB) detectors. With the GBM, the IPN will comprise 9 experimen…

astro-ph.HE2009

The Interplanetary Network Supplement to the HETE-2 Gamma-Ray Burst Catalog

K. Hurley, J. -L. Atteia, C. Barraud +43

Between 2000 November and 2006 May, one or more spacecraft of the interplanetary network (IPN) detected 226 cosmic gamma-ray bursts that were also detected by the FREGATE experimen…

astro-ph.HE2009★ 59 cited

A new analysis of the short-duration, hard-spectrum GRB 051103, a possible extragalactic SGR giant flare

K. Hurley, A. Rowlinson, E. Bellm +34

GRB 051103 is considered to be a candidate soft gamma repeater (SGR) extragalactic giant magnetar flare by virtue of its proximity on the sky to M81/M82, as well as its time histor…

astro-ph2005★ 598 cited

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…

astro-ph2002★ 90 cited

Discovery of GRB 020405 and its Late Red Bump

P. A. Price, S. R. Kulkarni, E. Berger +41

We present the discovery of GRB 020405 made with the Inter-Planetary Network (IPN). With a duration of 60 s, the burst appears to be a typical long duration event. We observed the…