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Dear ASCA users,

We have accepted a 10-ksec TOO observation  of the transient source
XTE J1723-376 and the observation is allocated on March 3, 1999.
This transient, discovered on January 25, is a rare transient with kHz 
QPO and its high state has been continuing with intensity of about 80 
mCrab on February 22. We attempt to refine its position and to get 
low energy spectrum with high resolution. The PI of the observation 
is Frank Marshall,  CoI  Craig Markwardt and Japanese CoIs are TBD.

F. Nagase
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A S C A     WEEKLY  OBSERVATION   PLAN
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#06: March  4 - 14, 1999			ver-2   (99/ 2/25)
(ISAS contact scientist: 	Y. Ueda	(ueda@astro.isas.ac.jp)
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Date	MNV	Target 		Tag. 	Exp.	Observation	PI or 
	start	name 		Cat.	(ks)	Cat.  Pri./TC	 ( PPI/Co-PI)
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3/ 4	 4:30	XTE J1723-376	Bin. 	10	TOO	1/Y	F. Marshall
									 
3/ 4	10:50	G156.2+5.6SE	SNR	40	MUJ	2/n	R. Petre
								/TBD
3/ 5	 7:20	G156.2+5.6W	SNR	40	MUJ	2/n	R. Petre
								/TBD
3/ 6	 2:40	1E161348 N3	SNR	20	MUJ	1/n 	E. Gotthelf
								/TBD
3/ 6	13:40	G350.0-1.8	SNR	30	JPN	2/n	M. Ozaki

3/ 7	 7:10	IC 443		SNR	60	JPN	2/n	K. Torii

3/ 8	19:20	Chamelleon III	Star	80	JPN	2/n	S. Yamauchi

3/10	16:10	GC Reg. N1	SNR	10	JPN	1/n	S. Yamauchi

3/10	22:20	GC Reg. N2	SNR	10	JPN	1/n	S. Yamauchi

3/11	 3:40	GC Reg. N3	SNR	10	JPN	1/n	S. Yamauchi

3/11	 8:20	GC Reg. N4	SNR	10	JPN	1/n	S. Yamauchi

3/11	14:30	GC Reg. N5	SNR	10	JPN	1/n	S. Yamauchi

3/11	20:30	GC Reg. N6	SNR	10	JPN	1/n	S. Yamauchi

3/12	 1:50	GC Reg. N7	SNR	10	JPN	1/n	S. Yamauchi

3/12	 6:40	GC Reg. N8	SNR	10	JPN	1/n	S. Yamauchi

3/12	12:40	GC Reg. N9	SNR	10	JPN	1/n	S. Yamauchi

3/12	19:10	GC Reg. N10	SNR	10	JPN	1/n	S. Yamauchi

3/12	23:50	Abell 3408	CG	60	JPN	1/n   	K. Hashimotodani

(3/14	15:10  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, 
MOT: Observatory Time (Calibration, maintenance), 
and TOO: Target of Opportunity