SUMMARY OF PROPOSAL 61226
TOKYO METROPOLITAN UNIVERSITY
TOKYO JAPAN 192-03
HACHIOJI-SHI
1-1, MINAMI-OSAWA
Tel: +81-426-77-2485 Fax: +81-426-77-2483
Medium: 4GBDAT
Subject: COSMIC X-RAY BACKGROUND DEEP SURVEYS AND OTHER
FOLLOW-UP OBSERVATION OF ULTRA DEEP ROSAT FIELD: THE LOCKMAN HOLE (II)
ABSTRACT
We propose 100 ks observation of the Lockman Hole, where the deepest ROSAT observations (PSPC: 207 ks, HRI: 1040 ks) exist. We plan to extend ASCA observation in both area and deepness to cover the ROSAT surveyed area (r < 18.5 arcmin). Lockman Hole is suitable for studying the origin of the CXB above 2 keV, because the soft X-ray catalogue with complete optical identification is available down to 5x10**-15 erg/s/cm2. Most sources detected with previous ASCA observations are already catalogued in the ROSAT paper (Hasinger 1997, submitted).
CO-INVESTIGATORS
CO-I NAME | INSTITUTE | COUNTRY |
---|
TAKAMITSU MIYAJI | A.I.P. | GERMANY |
GUENTHER HASINGER | A.I.P. | GERMANY |
YASUSHI OGASAKA | NASA/GSFC/JSPS | JAPAN |
KIYOSHI HAYASHIDA | OSAKA UNIVERSITY | JAPAN |
YOSHIHIRO UEDA | ISAS | JAPAN |
TADAYUKI TAKAHASHI | ISAS | JAPAN |
TSUNEO KII | ISAS | JAPAN |
HAJIME INOUE | ISAS | JAPAN |
KAZUO MAKISHIMA | UNIVERSITY OF TOKYO | JAPAN |
TORU YAMADA | TOHOKU UNIVERSITY | JAPAN |
TARGETS
TARGET NAME | PRI | RA | DEC | TIME | TC | OFF | GIS | SIS CNT | OBS |
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1)LOCKMAN HOLE | 2 | 163.0000 | 57.3600 | 100 ks | N | Y | P | 0.01000 | 1 |