ChaMPlane Observation: WIYN/Hydra
October 31, 2002
Here is a list of all the ChaMPlane Fields Observed with WIYN/Hydra
ChaMPlane WIYN Observation Field List
N Field RA Dec glong glat nH(e22) Mosaic Targets New-Old OptID
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1 GK PERSEI 03:31:12.00 +43:54:17.0 150.957 -10.104 0.236 kpno00 X Xo H M F all opt ha
2 GRO J0422+32 04:21:42.80 +32:54:27.0 165.880 -11.915 0.166 kpno00 X Xo H XoH M F all opt ha
3 NGC 1569 04:30:49.00 +64:50:54.0 143.683 11.241 0.224 kpno00 X Xo H M F all opt ha
4 3C 123 04:36:28.00 +29:37:49.0 170.526 -11.787 0.190 kpno01 X Xo H M F all opt ha
5 3C 129 04:49:19.20 +45:02:30.0 160.424 0.184 0.733 kpno01 X Xo H M F all opt ha
6 A0620-00 06:23:15.70 -00:18:20.7 209.958 -6.540 0.410 ctio01 X Xo H XoH M F all opt ha
7 MWC297 18:27:39.60 -03:49:52.0 26.803 3.526 0.492 ctio01 X Xo H M F H03 H05
8 SGR1900+14 19:07:14.30 +09:19:20.1 43.022 0.766 1.420 ctio01 X Xo H XoH M F H03 H05
9 B2224+65 22:25:52.40 +65:35:33.8 108.637 6.845 0.553 kpno01 X Xo H M F all opt ha
10 3EG J2227+6122 22:29:17.00 +61:19:00.9 106.711 3.006 0.995 kpno01 X Xo H M F all opt ha
11 G116.9+0.2 23:59:12.53 +62:24:00.0 116.943 0.184 0.670 kpno02 H M F all opt ha
12 G127.1+0.5 01:28:32.00 +63:06:34.0 127.113 0.539 0.938 kpno02 H M F all opt ha
13 G166.0+4.2 05:26:49.00 +42:57:19.0 166.131 4.338 0.488 kpno02 Xo H M F all opt ha
14 PSRJ0538+2817 05:38:25.10 +28:17:11.0 179.719 -1.686 0.613 kpno02 Xo H M F all opt ha
15 MADDALENACLOUD 06:49:05.50 -04:33:50.0 216.730 -2.600 0.803 kpno02 H M F all opt ha
16 M1-16 07:37:18.60 -09:38:48.0 226.800 5.626 0.305 kpno02 Xo H M F all opt ha
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Click a field name to see the color-magnitude diagram of that field with H-alpha and
Chandra sources marked.
Source lists:
X Chandra source optical counterparts.
NOTE: The purpose of this list is to provide the RA and Dec for
the Chandra optical counterparts. Some of the brighter optical
magnitudes (and Ha-R) may not be accurate due to saturation and
therefore large psf fit Chi^2.
Xo Chandra source optical counterparts.
This list is a subset of list X. It contains only those objects
with good psf fit and correct magnitudes from list X.
This list is sorted by the sigma of matching: sigma = match*3/err_3s
H Ha emission sources with Ha-R < -0.3 and SNR > 5.
(Ha-R < -0.35 and SNR > 10 for SGR1900+14)
XoH Chandra source optical counterparts with Ha emission.
The objects in this list are in both Xo and H.
M Ha emission sources with -0.3 < Ha-R < -0.2 and SNR > 5. Most of
them are probably M stars.
(-0.35< Ha-R < -0.25 and SNR > 10 for SGR1900+14)
F FOPS (field positioner) stars with 13 < R < 17.
H03 Ha emission sources with Ha-R < -0.3, regardless of SNR.
H05 Ha emission sources with Ha-R < -0.5, regardless of SNR.
Note: SGR1900+14 did not go very deep. It only has 3x4min R images
and one 25 min Ha image. So its color Ha-R is very noisy. Therefore
I raised the criteria to select its H and M list.
New-Old OptID: New-Old Optical ID matching lists.
all: matching lists for opt_all.rdb - all daophot output.
opt: matching lists for opt.rdb - stars selected with sharpness, chisqr and errors.
ha: matching lists for Ha emission objects.
Each matching list has three columns:
ID: new optical ID
IDo: old optical ID
match: matching distance between the new and old optical IDs, in arcsec.
ha lists also have new and old H-R magnitude and SNR.
Ping Zhao: zhao@cfa.harvard.edu