ChaMPlane Magellan/IMACS Observation Target Fields
MID Mosaic Field RA(J2000) Dec(J2000) l b NH(e22)
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30 kpno02 M116 07:37:16.19 -09:41:12.8 226.830 5.598 0.130
59 kpno04 OH231 07:42:13.33 -14:43:57.9 231.844 4.198 0.804
60 ctio05 PSR1046 10:47:58.55 -58:29:39.4 287.380 0.599 0.664
31 ctio03 MSH11 11:11:58.64 -60:41:34.6 291.054 -0.136 0.639
15 ctio01 NGC3603 11:15:52.55 -61:17:46.5 291.715 -0.523 14.958
32 ctio03 G292 11:19:46.34 -61:40:05.4 292.282 -0.707 2.171
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Mask RA(J2000) Dec(J2000) setup files mask finding X b f Xha b f Xhm b f Ha b f Hm b f Slit ---------------------------------------------------------------------------------------------------------------------------------------- M116A 07:37:14.848 -09:40:09.96 obs obw SMF mask det jpg ps 16 18.8 24.0 1 22.2 22.2 3 18.8 22.5 31 20.3 23.0 59 17.3 23.4 106 OH231Ad 07:42:18.444 -14:44:00.68 obs obw SMF mask det jpg ps 20 17.0 24.7 1 21.4 21.4 7 17.0 20.2 11 20.3 23.5 37 19.3 22.9 68 PSR1046A 10:48:27.552 -58:32:00.51 obs obw SMF mask det jpg ps 26 16.2 23.3 1 22.0 22.0 7 16.5 19.6 10 21.1 23.4 53 17.6 23.6 89 MSH11Ad 11:11:19.392 -60:41:55.90 obs obw SMF mask det jpg ps 31 16.5 22.5 3 16.5 19.7 1 17.3 17.3 42 18.8 21.9 13 19.6 22.6 86 NGC3603Ad11:15:14.609 -61:16:57.56 obs obw SMF mask det jpg ps 42 17.0 23.8 4 18.4 22.1 4 17.0 21.7 48 17.1 22.8 4 20.7 22.2 94 G292Ad 11:19:30.490 -61:27:47.15 obs obw SMF mask det jpg ps 32 15.0 23.5 2 15.0 19.8 3 19.0 22.3 27 20.5 22.8 28 19.8 23.4 87 ---------------------------------------------------------------------------------------------------------------------------------------- RA&Dec: center of the mask, telescope pointing. X: number of Chandra sources, priority -1. Xha: number of Chandra sources with Ha emission (H-R<-0.3 & SNR>5), priority -3. Xhm: number of Chandra sources with Hm emission (H-R<-0.2 & SNR>3), priority -2. Ha: number of non-Chandra Ha emission objects (H-R<-0.3 & SNR>5), priority 1. Hm: number of non-Chandra Hm emission objects (H-R<-0.2 & SNR>3), priority 2. b,f: bright and faint R limit of the group. slit: number of slits on the mask d: done (observed) All above are faint masks. Alignment stars are chosen from opt_p.rdb tables, 17 < R < 19. Mask musthave = -3
1. Take images of the masks at the same binning as is intended for the nighttime observations. These are usually exposures of 1-2 seconds taken with the lower-light-level quartz lamp controlled by a power supply at the base of the telescope.
Astronomical twilight: 21:16 - 4:34 duration 7h18m Observe three mask each night: 3 x 146min = 438m = 7h18m Using 2x2 binning saves disk space (not so important) but also readout time.Here is an observing elevation chart for this run on January 23, 2008.

Here is an observing almanac made for this run.
Here is the Las Campanas Observatory 2008 Ephemeris.
Ping Zhao 1/2/2008