# Template tunable parameter file for reducing survey scans against UCAC.

rwindowBig     15.0             # Initial big row match-up window (arcsecs).
cwindowBig     15.0             # Initial big column match-up window (arcsecs).
rwindowSmall    3.0             # Final small row match-up window (arcsecs).
cwindowSmall    3.0             # Final small column match-up window (arcsecs).
rwindowTiny     0.5             # Repeat row match-up window (arcsecs).
cwindowTiny     0.5             # Repeat column match-up window (arcsecs).

frameLogUpdate    1             # Update boresight ra and dec values from the
                                # idFrameLog files, before calculating initial
                                # guesses at CMP positions for initial matching

# The following three parameters transform the color in the known object
# catalog for primary match into r'-i'.  Thus:
#   r'-i' = catColor0 + catColor1 * color + catColor2 * color * color...
# The samples transform B-V to r'-i' for the ACT catalog:
catColor0	 0		# Zero-order term in color transform
catColor1	 0		# First-order term in color transform
catColor2	 0		# Second-order term in color transform
catColor3	 0		# Third-order term in color transform

magDiff 1.5

# Don't use catalog stars with ra or dec errors larger than the following
# specified value.
catErrMax         60            # Maximum error in ra or dec for catalog
				# star to use (mas)

primAll         2               # 0=process astrometrics against sky,
                                #   photometrics against secondary catalog;
				# 1=process all CCDs directly against the sky
				# 2=process r' against the sky, fitting all
				#   together, and remaining photometrics
				#   against the secondary catalog;
				# 3=process r' against the sky, fitting each
				#   separately, and remaining photometrics
				#   against the secondary catalog

meansWindow(prim)  30		# Running means window for primary match(stars)
meansWindow(astro) 0		# Running means window for astro chips match
				# (stars)

splineLength(bore) 0		# Number of frames per polynomial in primary
				# match, fitting all r' CCDs together
				# (0=no spline fit)
splineLength(prim) 5		# Number of frames per polynomial in primary
				# match, fitting each r' CCD separately
				# (0=no spline fit)
splineLength(astro) 0		# Number of frames per polynomial when matching
				# astrometric CCDs against r' CCD
				# (0=no spline fit)