activity
20062010
most citedA Comprehensive Study of Short Bursts from SGR 1806-20 and SGR 1900+14 Detected by HETE-2

50 citations · 152 across the 10 of their papers we have counts for

collaborators

10 papers

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.HE2010★ 16 cited

Spectral Lag Relations in GRB Pulses Detected with HETE-2

M. Arimoto, N. Kawai, K. Asano +36

Using a pulse-fit method, we investigate the spectral lags between the traditional gamma-ray band (50-400 keV) and the X-ray band (6-25 keV) for 8 GRBs with known redshifts (GRB 01…

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-ph2008

Rising optical afterglows seen by TAROT

B. Gendre, A. Klotz, G. Stratta +8

We present the multi-wavelength study of those gamma-ray bursts observed by TAROT. These events are characterized by the presence at early time of a rising in their optical light c…

astro-ph2008★ 32 cited

Early emission of rising optical afterglows: The case of GRB 060904B and GRB 070420

A. Klotz, B. Gendre, G. Stratta +8

We present the time-resolved optical emission of gamma-ray bursts GRB 060904B and GRB 070420 during their prompt and early afterglow phases. We used time resolved photometry from o…

astro-ph2008★ 17 cited

Multiple Component Analysis of Time Resolved Spectra of GRB041006: A Clue to the Nature of Underlying Soft Component of GRBs

Yuji Shirasaki, Atsumasa Yoshida, Nobuyuki Kawai +30

GRB 041006 was detected by HETE-2 at 12:18:08 UT on 06 October 2004. This GRB displays a soft X-ray emission, a precursor before the onset of the main event, and also a soft X-ray…