imstar(1)
Find stars in FITS and IRAF image files imstar [options] [FITS or IRAF filename] or [@file of image file names] Coordina
Description
imstar
Name
imstar - Find stars in FITS and IRAF image files
Synopsis
imstar [options] [FITS or IRAF filename] or [@file of image file names]
Description
Options
<hh:mm:ss> <dd:mm:ss> [J2000, B1950]
Coordinates for center (or reference pixel if -x is used).
-a <angle>
Image rotation angle in degrees (default 0). If multiple of 90, rotate image before search and set WCS angle to zero; if not, put in WCS.
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-b |
Output B1950 (FK4) coordinates (default=image equinox) |
-d <catalog name>
Read this DAOFIND style catalog of X, Y, and magnitude instead of searching for stars in the image. The format is simply white-space-separated numbers on a line, with # at the beginning of comment lines.
-e <num>
Number of pixels to ignore around image edge
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-f |
Write a simple ASCII catalog file instead of tab table or DAOFIND format (number RA DEC mag ... per line, with two lines of header info) | ||
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-h |
Print heading, else do not |
-i <num>
Minimum peak value for star in image (<0=-sigma) Setting this to reject all but 10-15 stars is a good way to speed up the star-finding process. If num is less than zero, the minimum peak is -num image pixel standard deviations. Setting this number rejects faint stars early in the selection process for a significant saving in computing time.
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-j |
Output J2000 (FK5) coordinates (default=image equinox) | ||
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-k |
Print each star as it is found for debugging | ||
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-l |
Reflect the image left <-> right before rotating (-a) and searching for stars. |
-m <magnitude>
Magnitude offset
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-n |
Number of brightest stars to print | ||
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-o |
Output star list in DAOFIND format. The first three numbers on each line of the output file are X, Y, and magnitude, separated by one or more blanks or a tab. Lines beginning with # are ignored. |
-p <num>
Plate scale in arcsec per pixel (default 0)
-q <c|d|o|s|x|v|+>
Output region file shape for SAOimage (default o) Characters mean: c>ross, d>iamond, s>quare, o>circle, x=X, v>ary with GSC type, +>cross.
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-r |
Maximum radius for star in pixels | ||
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-s |
Sort by RA instead of flux | ||
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-t |
Output in Starbase tab table format | ||
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-v |
Verbose listing of processing intermediate results | ||
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-w |
Write output to a file in addition to standard out. If DAO format (-o), create the name by adding .dao to the image file name. If Starbase format (-t), create the name by adding .tab to the image file name. If ASCII format (-f), create the name by adding .stars to the image file name. |
-x <X> <Y>
X and Y coordinates of reference pixel (if not in header or image center)
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-z |
Use AIPS classic projection code (for "-SIN", "-TAN", "-ARC", "-NCP", "-GLS", "-MER", "-AIT" and "-STG" only) instead of WCSLIB proposed standard projection code. |
Web Page
http://tdc-www.harvard.edu/software/wcstools/imstar/
Author
Jessica Mink, SAO (jmink@cfa.harvard.edu)