Back to Search Start Over

GRB observations with the HETE soft X-ray cameras

Authors :
Vanderspek, R.
Villaseñor, J.
Doty, J.
Jernigan, J. G.
Levine, A.
Monnelly, G.
Ricker, G. R.
Vanderspek, R.
Villaseñor, J.
Doty, J.
Jernigan, J. G.
Levine, A.
Monnelly, G.
Ricker, G. R.
Source :
Astronomy and Astrophysics. Supplement Series; September 1999, Vol. 138 Issue: 3 p565-566, 2p
Publication Year :
1999

Abstract

The High Energy Transient Explorer, scheduled to be launched in late 1999 or early 2000, will carry a pair of Soft X-ray Cameras (SXC), capable of localizing the X-ray counterparts of GRBs with unprecedented precision. Each SXC consists of a pair of large-format CCDs behind a 1-D coded aperture: the two SXCs are oriented orthogonal to each other to permit two-dimensional image reconstruction. The SXCs on HETE will be able to localize bright X-ray afterglows to $<20''$precision within seconds of burst onset. The coordinates of detected bursts will be distributed immediately to ground-based observers and to the GCN via the HETE Burst Alert System.

Details

Language :
English
ISSN :
03650138
Volume :
138
Issue :
3
Database :
Supplemental Index
Journal :
Astronomy and Astrophysics. Supplement Series
Publication Type :
Periodical
Accession number :
ejs53389806
Full Text :
https://doi.org/10.1051/aas:1999354