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ASCA weekly
Dear ASCA users,
An ASCA TOO observation of an X-ray transient, XTE J2012+381, an
outburst of which was discovered with RXTE/ASM, was proposed. We
decided to perform an ASCA TOO observation during the span on May 29 6:00
to May 30 4:30 (UT). The source is suspected to be a black hole candidate
and it may be still in the intesity incleasing phase at the time of the ASCA
observation. The PI of the TOO is N. White, US CoIs; TBD, Janese CoIs;
F. Nagase, Y. Ueda, T. Dotani, and TBA. The cluster, MS 1910+6736, once
installed in the span is carried over and will be ischeduled in the next
visible window.
In the re-servay project of the central part (Y. Ueda) of the previous
"Large Sky Survey" region, the pointing numbers were reduced from 10
pointings to 4 pointings to get deeper exposure in each field.
F. Nagase
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A S C A WEEKLY OBSERVATION PLAN
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May 28 - June 9, 1998, ver-3 (98/ 5/29)
(ISAS contact scientist: T. TAMURA (ttamura@astro.isas.ac.jp)
-----------------------------------------------------------------------------
Date MNV Target Tag. Exp. Observation PI or
start name Cat. (ks) Cat. Pri./TC ( PPI/Co-PI)
-----------------------------------------------------------------------------
5/28 3:20 5C12_75 CG 40 JPN 2/n K. Hayashida
(AO-5 Supplemental)
5/29 6:00 XTE J2012+381 Bin. 40 TOO 1/Y N. White
5/30 4:30 IRAS 00198-7926 AGN 100 JPN 2/n Y. Ogasaka
6/ 1 20:20 CENT #1 CXB 50 JPN 1/n Y. Ueda
6/ 3 5:30 CENT #2 CXB 50 JPN 1/n Y. Ueda
6/ 4 13:20 CENT #3 CXB 45 JPN 1/n Y. Ueda
6/ 5 16:20 CENT #4 CXB 55 JPN 1/n Y. Ueda
6/ 7 0:30 H1426+428 AGN 40 US 2/n R. Sambruna
6/ 8 0:30 IRAS12397+3333 AGN 40 ESJ 2/n D. Grupe
(6/ 9 0:20, MNV to next target)
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(Note) Obs. Cat. JPN: Japan time, US: US time, JUS: Japan-US Collaboration,
USJ: US-Japan Collaboration, MJU: Merged Japan-US (PPI=Japan),
MUJ: Merged US-Japan (PPI=US), ESJ: ESA-Japan Program,
OT: Observatory Time (Calibration, maintenance and TOO)