Once the object list has been calibrated against the USNO A2.0 catalog, we are in a position to know how to map the image coordinates to the sky, and we can fill in all of the image file headers. The following fields now have meaningful values that define a (very rough) WCS rotation matrix to perform this conversion: PC001001, PC002002, PC001002, and PC002001. These numbers are used by ds9 to calculate world coordinate system units for display, but are not accurate enough for real analysis.
A cobj FITS file has a primary header and two data extensions. The primary header is taken directly from the corrected image. The first data extension contains the calibrated object list. The second data extension contains the ``calibration structure,'' or ``cal'' structure.
The calibrated object list at extension 1 is an array of structures, one element per object, each element of which contains the following fields:
RA Right Ascention (deg)
DEC Declination (deg)
X Horizontal Pixel coordinate
Y Verticle Pixel coordinate
M Calibrated magnitude
MERR Uncertainty in above
FLAGS Same as in sobj file
RFLAGS Additional ROTSE flags (See Table C.2)
The cal structure at extension 2 contains a single structure with much information. The bulk of the cal structure consists of the corrected image header keywords converted from ASCII to a binary structure. In addition are several important keywords from the sobj header. Finally are calibration diagnostic values described here:
BADPIXFILE The name of the bad pixel file
NMATCH The number of matched objects
OFFSET_X
OFFSET_Y
POS_SIGMA The RMS error in position
RA_LOW Image range on sky
RA_HIGH
DEC_LOW
DEC_HIGH
ZP_OFFSET Magnitude offset
ZP_SIGMA Uncertainty in offset
M_LIM Limiting magnitude
FNAME Name of file
RAC Coordinate of center
DECC
KX Third order rotation matrix
KY to convert coords
SAT_MAG Saturation magnitude
NOBJ_BADPIX Objects that fall on bad pixels
SKY 6464 array for sky bkgd
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