Free Access
Issue
Astron. Astrophys. Suppl. Ser.
Volume 138, Number 3, September 1999
Gamma-Ray Bursts in the Afterglow Era Contents Rome, November 3-6, 1998
Page(s) 563 - 564
DOI https://doi.org/10.1051/aas:1999353
Published online 15 September 1999
DOI: 10.1051/aas:1999353



Astron. Astrophys. Suppl. Ser. 138, 563-564

Wide-field X-ray Monitor on HETE-2

N. Kawai1 - M. Matsuoka1 - A. Yoshida1 - Y. Shirasaki1 - M. Namiki1 - K. Takagishi2 - M. Yamauchi2 - I. Hatsukade2 - E.E. Fenimore3 - M. Galassi3

Send offprint request: N. Kawai


1 - RIKEN, The Institute of Physical and Chemical Research, 2-1, Hirosawa, Wako, Saitama 351-0198, Japan
e-mail: nkawai@postman.riken.go.jp
2 - Miyazaki University, Faculty of Engineering, Gakuen-kihanadai-nishi, Miyazaki 880-2155, Japan
3 - Los Alamos National Laboratory, MS D436, Los Alamos NM87545, U.S.A.

Received January 21; accepted March 10, 1999

Abstract:

The Wide-field X-ray Monitor on HETE-2 consists of four Xe-filled 1-D position-sensitive proportional counters. It is sensitive to X-rays between 2 keV and 25 keV, and is designed to localize gamma-ray bursts in real time with $\sim10^{\prime}$ accuracy. The design and basic characteristics of the detectors are presented.

Key words: instrumentation: detectors -- gamma-rays: bursts -- X-rays: general

Copyright The European Southern Observatory (ESO)

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