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Timestamp:
Nov 2, 2005, 3:25:26 PM (21 years ago)
Author:
Paul Price
Message:

Fixed definition of pmSubtractBias.

File:
1 edited

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  • trunk/doc/modules/ModulesSDRS.tex

    r5378 r5461  
    1 %%% $Id: ModulesSDRS.tex,v 1.65 2005-10-19 03:24:53 eugene Exp $
     1%%% $Id: ModulesSDRS.tex,v 1.66 2005-11-03 01:25:16 price Exp $
    22\documentclass[panstarrs,spec]{panstarrs}
    33
     
    877877Overscan subtraction is controlled by the \code{overscan} boolean.  If
    878878it is \code{true}, then overscan subtraction is performed.  The
    879 prescan and/or overscan regions to be used are specified in
    880 \code{in->bias} (a linked list of subimages).  These shall be reduced
    881 to a single vector (in the dimension specified by \code{CELL.READDIR},
     879prescan and/or overscan regions to be used are specified in by
     880\code{CELL.BIASSEC} (accessed via the parent of the \code{pmReadout};
     881a linked list of \code{psRegion}s).  These shall be reduced to a
     882single vector (in the dimension specified by \code{CELL.READDIR},
    882883which is accessed via the parent of the \code{pmReadout}).
    883884
     
    932933then no fit shall be performed to the overscan.
    933934
    934 A bias frame shall be subtracted pixel-by-pixel from the input image
    935 if \code{bias} is non-NULL.  If \code{dark} is non-\code{NULL}, then
    936 the dark image, scaled by the ratio of dark times (from
     935A \code{bias} frame shall be subtracted pixel-by-pixel from the input
     936image if \code{bias} is non-NULL.  If \code{dark} is non-\code{NULL},
     937then the dark image, scaled by the ratio of dark times (from
    937938\code{CELL.DARKTIME}) shall be subtracted pixel-by-pixel from the
    938 input image.  Note that the input image,
    939 \code{in}, and the \code{bias} and \code{dark} frames need not be the
    940 same size, but the function shall use the offsets in the image
    941 (\code{in->x0} and \code{in->y0}) to determine the appropriate offsets
    942 to obtain the correct pixel on the \code{bias}.  In the event that the
    943 \code{bias} image is too small (i.e., pixels on the input image refer
    944 to pixels outside the range of the \code{bias} image), the function
    945 shall generate an error.  Any pixels masked in the \code{bias} or
     939input image.  The full-frame subtractions (both bias and dark) should
     940only be performed on the image region specified by
     941\code{CELL.TRIMSEC}.  Note that the input image, \code{in}, and the
     942\code{bias} and \code{dark} frames need not be the same size, but the
     943function shall use the offsets in the image (\code{in->x0} and
     944\code{in->y0}) to determine the appropriate offsets to obtain the
     945correct pixel on the \code{bias}.  In the event that the \code{bias}
     946image is too small (i.e., pixels on the input image refer to pixels
     947outside the range of the \code{bias} image), the function shall
     948generate an error.  Any pixels masked in the \code{bias} or
    946949\code{dark} shall also be masked in the output.  The bias and dark
    947950images may be copied to the same type as the input image if required.
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