postscript and txt
ChaMPlane WIYN Observation Field List August 3-7, 2002
Pri Field RA Dec glong glat nH(e22) Mosaic Targets
-------------------------------------------------------------------------------------------
1 B2224+65 22:25:52.40 +65:35:33.8 108.637 6.845 0.553 kpno00 X Xo H M F
2 3EG J2227+6122 22:29:17.00 +61:19:00.9 106.711 3.006 0.995 kpno01 X Xo H M F
3 SGR1900+14 19:07:14.30 +09:19:20.1 43.022 0.766 1.420 ctio01 X Xo H XoH M F
4 MWC297 18:27:39.60 -03:49:52.0 26.803 3.526 0.492 ctio01 H M F
-------------------------------------------------------------------------------------------
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 the correct magnitudes from list X.
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.
Only SGR1900+14 has this list. Other fields don't have
Chandra source with Ha emission.
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.
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.
postscript and
txt
Ping