I. Field List

          ChaMPlane WIYN Observation Field List    August 3-7, 2002
	                                                                  
Pri Field         RA           Dec            glong     glat nH(e22) Mosaic     Targets
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1  SGR1900+14     19:07:14.30  +09:19:20.1   43.022    0.766  1.420  ctio01  X Xo H XoH M F 
2  3C129          04:49:19.20  +45:02:30.0  160.424    0.184  0.733  kpno01  X Xo H     M F 
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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 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.

II. Observing Chart

postscript and txt

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