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AO3 observation status
Dear ASCA users,
I have reviewed current status of ASCA observation for AO3. Followins are
the list of
1. Targets to be schedule for Dec 1995,
2. XTE targets that are delayed until next year,
3. Targets that were removed from the long-term schedule, and
4. Targets that need additional observation.
Observations of targets in Table 1 will be scheduled in the first two weeks
of December. Supplemental observations for targets in Table 4 will be allocated
in the earliest opportunity of next window.
Regards,
F. Nagase
--------------------------------------------------------------------------------
1. Targets to be schedule for Dec 1995:
---------------------------------------
Seq # Target Cat Pri R.A. Dec. Exp TC Obs SIS P.I. Sun
(deg) (deg) (ks) Cat cts <
-------- -------------- --- --- -------- -------- ---- - --- ---- -------- ---
73037000 PG_1148+549 AGN 3 177.8333 54.6256 40.0 n JPN 0.04 TERASHIM 102
73084000 CTA_102 AGN 2 338.1500 11.7308 20.0 n USJ 0.5 MADEJSKI 105
73028000 MKN477 AGN 2 220.1585 53.5044 40.0 n JPN 0.05 AWAKI 80
73027000 NGC5005 AGN 2 197.7383 37.0575 40.0 n JPN 0.05 AWAKI 78
73062000 IRAS_00317-214 AGN 3 8.5571 -21.4386 40.0 n US 0.09 HELFAND 104
43029000 CYG_X-2 BIN 2 326.1713 38.3217 40.0 y USJ 250. VRTILEK 108
23013000 CQ_CEP STAR 2 339.2065 59.9065 40.0 y JPN 0.2 MAEDA 106
83027000 J1888.16CL CG 3 14.2340 -27.6748 20.0 n JPN .001 TAWARA 100
83025000 HCG42 CG 2 150.0577 -19.6365 40.0 n JPN 0.5 SAKIMA 98
73050000 HE_1029-1401 AGN 2 157.9750 -14.2808 40.0 n ESJ 0.2 SMITH 94
63012000 NGC5033 GAL 2 198.3659 36.5944 40.0 n JPN 0.2 TERASHIM 83
------------------------------------------------------------------------------
2. XTE targets that are delayed until next year:
------------------------------------------------
Seq # Target Cat Pri R.A. Dec. Exp TC Obs SIS P.I. Sun
(deg) (deg) (ks) Cat cts <
-------- -------------- --- --- -------- -------- ---- - --- ---- -------- ---
43030000 LMC_X-4 BIN 1 83.2042 -66.3706 50.0 y USJ 4.0 VRTILEK 92
33011000 BG_CMI CV 2 112.8708 9.9394 40.0 y USJ 0.5 MUKAI 103
33011010 BG_CMI CV 2 112.8708 9.9394 40.0 y USJ 0.5 MUKAI 103
--------------------------------------------------------------------------------
3. Targets that were removed from the long-term schedule:
---------------------------------------------------------
Seq # Target Cat Pri R.A. Dec. Exp TC Obs SIS P.I. Sun
(deg) (deg) (ks) Cat cts <
-------- -------------- --- --- -------- -------- ---- - --- ---- -------- ---
53000000 G-LONGITUDE_32 SNR 3 234.6300 -55.5100 30.0 n JPN 0.05 MAKISHIM 97
11010000 N132D GAL 1 81.2600 -69.6420 40.0 n JPN 0.0 ASCA_TEA 92
--------------------------------------------------------------------------------
* Makashima's Priority C target was dropped in favor of TOO NOVA SCO (Aug 1995).
* N132D was not needed for calibration.
* In addition to the avove two drop-out, the exposure time for Koyama's Galactic
Ridge survey project was reduced from 50 ksec to 35 ksec to allocate the
rest to TOO observation.
4. Targets that need additional observation to supply the insufficient exposure:
--------------------------------------------------------------------------------
Target Cat. Pri Observed Exposuretime (ksec) P.I.
approved achieved tobe added
--------- ---- ---- -------- -------- -------- ---------- ----------------
Q1508+5714 AGN 1 95/ 3/ 2 80 38 26 D. Helfand
SN1993J SNR 2 95/ 4/ 1 50 23 27 H. Inoue
3C 303 AGN 1 95/ 5/21 40 21 19 H. Inoue
XY Ari CV 1 95/ 8/ 6 40 34 6 E. Schlegel
V773 Tau Star 2 95/ 9/16 40 26 14 S. Skinner
ESO 103-G35 AGN 1 95/ 9/26 19 4 19 K. Leighly
-----------------------------------------------------------------------------------------
* These supplements are based on the survay of observation log between 95 March 1 to
95 October 6. A few more supplements will be added later for the AO3 observations
between October 7 and end of AO3 (middle Decmber), since already we have
information of emergent cancellation of scheduled DNS telemetry down-link.
* ESO 103-G35 was a priority-A target of AO2 of approved time 40 ksec. Unfortunately,
we met trouble again in the supplement observation, and added exposure time
was very small and useless. A full re-observation for the supplement will be
planned again in the next window.
---------------------------------------------------------------------------------------fin