# Template tunable parameter file for reducing calibration scans # against UCAC or FASTT. magDiff 2. # Maximum allowed difference in magnitude # when matching by position # The following two parameters control how many times the fits are iterated # either re-rejecting outliers or re-matching nClipIters 3 # Number of times to clip and fit nMatchIters 1 # Number of times to match and fit # 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 # Don't use catalog stars with ra or dec errors larger than the following # specified value. catErrMax 100 # Maximum error in ra or dec for catalog # star to use (mas) primAll 1 # 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) 0 # Running means window for primary match(stars) meansWindow(astro) 0 # Running means window for astro chips match # (stars) meansWindow(photo) 0 # Running means window for photo 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) 0.3333 # 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) splineLength(photo) 0 # Number of frames per polynomial when matching # photometric CCDs against r' CCD # (0=no spline fit) badCCDs # List of bad CCDs; don't use their stars when # creating the secondary standard star catalog