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Дата индексирования: Mon Apr 11 01:22:56 2016
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WFPC2 Drizzle Cookbooks
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Hubble Space Telescope
WFPC2 Drizzle Cookbooks

MultiDrizzle parameters with descriptions and default values

input = "*flt.fits"     Input files (name, wild-card and suffix, or @list)
      (output = "")             Rootname for output drizzled products
    (mdriztab = no)             Use Multidrizzle parameter file specified in header?
    (refimage = "")             
     (runfile = "")             File for logging the script commands
 (workinplace = no)             Work on input files in place? (NOT RECOMMENDED)
   (updatewcs = yes)            Update the WCS keywords?
      (coeffs = "header")       Use header-based distortion coefficients?
     (context = yes)            Create context image during final drizzle?
       (clean = no)             Remove temporary files?
       (group = "")             
          (ra = )               right ascension output frame center in decimal degrees
         (dec = )               declination output frame center in decimal degrees
       (build = yes)            Create multi-extension output file?
   (shiftfile = "")             Shiftfile name
  (staticfile = "")             Name of (optional) input static bad-pixel mask
                                
                                STEP 1: STATIC MASK
      (static = yes)            Create static bad-pixel mask from the data?
  (static_sig = 4.0)            Sigma*rms below mode to clip for static mask
                                
                                STEP 2: SKY SUBTRACTION
      (skysub = yes)            Perform sky subtraction?
    (skywidth = 0.1)            Bin width for sampling sky statistics (in sigma)
     (skystat = "median")       Sky correction statistics parameter
    (skylower = INDEF)          Lower limit of usable data for sky (always in electrons)
    (skyupper = INDEF)          Upper limit of usable data for sky (always in electrons)
     (skyclip = 5)              Number of clipping iterations
   (skylsigma = 4.0)            Lower side clipping factor (in sigma)
   (skyusigma = 4.0)            Upper side clipping factor (in sigma)
     (skyuser = "")             KEYWORD indicating a sky subtraction value if done by user.
                                
                                STEP 3: DRIZZLE SEPARATE IMAGES
(driz_separat = yes)            Drizzle onto separate output images?
(driz_sep_out = )               Size of separate output frame's X-axis (pixels)
(driz_sep_out = )               Size of separate output frame's Y-axis (pixels)
(driz_sep_ker = "turbo")        Shape of kernel function
(driz_sep_wt_ = "exptime")      Weighting factor for input data image
(driz_sep_sca = INDEF)          Absolute size of output pixels in arcsec/pixel
(driz_sep_pix = 1.0)            Linear size of drop in input pixels
(driz_sep_rot = INDEF)          Position Angle of drizzled image's Y-axis w.r.t. North (degrees)
(driz_sep_fil = "INDEF")        Value to be assigned to undefined output points
(driz_sep_bit = 0)              Integer mask bit values considered good
                                
                                STEP 4: CREATE MEDIAN IMAGE
      (median = yes)            Create a median image?
(median_newma = yes)            Create new masks when doing the median?
(combine_type = "minmed")       Type of combine operation
(combine_nsig = "4 3")          minmed: Significance for accepting minimum instead of median
(combine_nlow = 0)              median|minimum: Number of low pixels to reject
(combine_nhig = 1)              median|minimum: Number of high pixels to reject
(combine_lthr = "INDEF")        median|minimum: Lower threshold for clipping input pixel values
(combine_hthr = "INDEF")        median|minimum: Upper threshold for clipping input pixel values
(combine_grow = 1)              minmed: Radius (pixels) for neighbor rejection
                                
                                STEP 5: BLOT BACK THE MEDIAN IMAGE
        (blot = yes)            Blot the median back to the input frame?
 (blot_interp = "poly5")        Interpolant (nearest,linear,poly3,poly5,sinc)
 (blot_sinscl = 1.0)            Scale for sinc interpolation kernel
                                
                                STEP 6: REMOVE COSMIC RAYS WITH DERIV, DRIZ_CR
     (driz_cr = yes)            Perform CR rejection with deriv and driz_cr?
(driz_cr_corr = no)             Create CR cleaned _cor file and a _crmask file?
 (driz_cr_snr = "3.5 3.0")      Driz_cr.SNR parameter
(driz_cr_grow = 1)              Driz_cr_grow parameter
(driz_cr_cteg = 0)              Driz_cr_ctegrow parameter
(driz_cr_scal = "1.2 0.7")      Driz_cr.scale parameter
                                
                                STEP 7: DRIZZLE FINAL COMBINED IMAGE
(driz_combine = yes)            Perform final drizzle image combination?
(final_wht_ty = "EXP")          Type of weighting for final drizzle
 (final_outnx = )               Size of FINAL output frame X-axis (pixels)
 (final_outny = )               Size of FINAL output frame Y-axis (pixels)
(final_kernel = "square")       Shape of kernel function
(final_wt_scl = "exptime")      Weighting factor for input data image
 (final_scale = INDEF)          Absolute size of output pixels in arcsec/pixel
(final_pixfra = 1.0)            Linear size of drop in input pixels
   (final_rot = 0.0)            Position Angle of drizzled image's Y-axis w.r.t. North (degrees)
(final_fillva = "INDEF")        Value to be assigned to undefined output points
  (final_bits = 0)              Integer mask bit values considered good
 (final_units = "cps")          Units for final drizzle image (counts or cps)
                                
                                OVERRIDE DEFAULT INSTRUMENT PARAMETERS
        (gain = )               Detector gain in electrons per count
   (gnkeyword = )               Detector gain keyword in header
     (rdnoise = )               Detector read noise in electrons
   (rnkeyword = )               Detector read noise keyword in header
     (exptime = )               Exposure time in seconds
  (expkeyword = )               Exposure time keyword in header
       (crbit = )               Bit value for CR ident. in DQ array
        (mode = "al")