IMMATCH(1)

πŸ’– IMMATCH β€” the matchmaking era πŸ’–

okay so bestie, pull up a chair πŸͺ‘βœ¨ this one is immatch, and it lives in section 1 of the user commands manual (the "stuff you type at a shell" section, iykyk). Her whole thing? AME. That's the name, that's the gig, that's the vibe. πŸ‘‘


✨ SYNOPSIS ✨

[-vl] [-m mag] [-n frac] [-s mode] [-g class] [-h maxref] [-i peak]

🌸 DESCRIPTION 🌸

so what does she do, you ask? πŸ¦‹ she matches a catalog to the stars she finds in your image, using the WCS baked into the image file. literally the glow-up pipeline from "random pixels" to "I know exactly which star you are."

here's the fuller shape of the invocation, no cap:

[-c catalog] [-p scale] [-b ra dec] [-j ra dec] [-r deg] [-t tol]
[-x x y] [-y frac] FITS or IRAF file(s)

and now the flags, one by one, because we do not skip πŸ’…:

  • -a ang β€” initial rotation angle in degrees (default 0)
  • -b β€” initial center given as B1950 (FK4) RA and Dec
  • -c cat β€” the reference catalog (gsc, uac, ujc, tab table file
  • -d cat β€” use the following DAOFIND output catalog instead of doing a search
  • -f β€” write the output as X Y RA Dec, instead of N RA Dec X Y
  • -g num β€” Guide Star Catalog class (-1=all, 0, 3 (default -1
  • -h num β€” maximum number of reference stars to use (10-200, default 25
  • -i num β€” minimum peak value for a star in the image (<0=-sigma)
  • -j β€” initial center given as J2000 (FK5) RA and Dec
  • -k β€” which magnitude to use (1 to nmag)
  • -l β€” reflect left<->right before rotating and fitting
  • -mx m1[,m2] β€” initial reference catalog magnitude and limits
  • -p num β€” initial plate scale in arcsec per pixel (default 0)
  • -q β€” fit the image to catalog magnitude polynomial(s)
  • -r ang β€” rotation angle in degrees before fitting (default 0)
  • -s frac β€” use this fraction extra stars (default 1.0)
  • -t tol β€” offset tolerance in pixels (default 20)
  • -u num β€” USNO catalog single plate number to accept
  • -v β€” verbose
  • -w β€” rotate the image WCS with the image
  • -x x y β€” X and Y coordinates of the reference pixel (default is center)
  • -y num β€” multiply image dimensions by this for the search (default is 1)
  • -z β€” use AIPS classic projections instead of WCSLIB
heads up bestie 🫢 if you're coming from the synopsis and wondering about -m mag, -n frac and -s mode β€” those are hanging out up there in the usage line, and -s shows up down here as frac. just the way she's written. copy it exactly, don't freestyle. πŸŽ€

and that's the whole page, fr fr. she's short but she's doing a LOT. 🌈

source/version: immatch EB_SOURCE Β· February 2026 β€” go match some stars, you absolute icon πŸ‘‘πŸ’œ

πŸ“¦ where this page comes from