activity
20012004
most citedOn The Spectrum and Spectropolarimetry of Type Ic Hypernova SN 2003dh/GRB 030329

114 citations · 162 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2004★ 6 cited

Global Characteristics of X-Ray Flashes and X-Ray-Rich GRBs Observed by HETE-2

T. Sakamoto, D. Q. Lamb, C. Graziani +35

We describe and discuss the global properties of 45 gamma-ray bursts (GRBs) observed by HETE-2 during the first three years of its mission, focusing on the properties of X-Ray Flas…

astro-ph2003★ 114 cited

On The Spectrum and Spectropolarimetry of Type Ic Hypernova SN 2003dh/GRB 030329

K. S. Kawabata, J. Deng, L. Wang +32

Spectroscopic and spectropolarimetric observations of SN 2003dh/GRB 030329 obtained in 2003 May using the Subaru 8.2 m telescope are presented. The properties of the SN are investi…

astro-ph2002

The E-peak distribution of the GRBs detected by HETE FREGATE instrument

C. Barraud, J. L. Atteia, J. F. Olive +1

The FREGATE gamma ray detector of HETE-2 is sensitive to photons between 6 and 400 keV. This sensitivity range, extended towards low energies, allows us to explore the emission of…

astro-ph2002★ 1 cited

FREGATE observation of a strong burst from SGR1900+14

J-F. Olive, K. Hurley, J-P. Dezalay +7

After a long period of quiescence, the soft gamma repeater SGR1900+14 was suddenly reactivated on April 2001. On July 2, 2001, a bright flare emitted by this source triggerred the…

astro-ph2002

GRB010921: Localization and Observations by the HETE Satellite

G. Ricker, K. Hurley, D. Lamb +36

On September 21 at 18950.56 SOD (05:15:50.56) UT the FREGATE gamma-ray instrument on the High Energy Transient Explorer (HETE) detected a bright gamma-ray burst (GRB). The burst wa…

astro-ph2001★ 41 cited

Detection of Pulsed X-ray Emission from The Fastest Millisecond Pulsar PSR B1937+21 with ASCA

M. Takahashi

We have detected pulsed X-ray emission from the fastest millisecond pulsar known, PSR B1937+21 (P=1.558 msec), with ASCA. The pulsar is detected as a point source above …