Provided by: gnuastro_0.11-1build1_amd64 
NAME
MakeCatalog - Make a catalog from labeled input images
SYNOPSIS
astmkcatalog [OPTION...] ASTRdata
DESCRIPTION
MakeCatalog is part of GNU Astronomy Utilities 0.11. MakeCatalog will create a catalog from an input,
labeled, and noise images.
For more information, please run any of the following commands. In particular the second contains a very
comprehensive explanation of MakeCatalog's invocation: expected input(s), output(s), and a full
description of all the options.
All options and their values:
$ astmkcatalog -P
Inputs/Outputs and options:
$ info astmkcatalog
Full section in manual/book:
$ info MakeCatalog
Full Gnuastro manual/book:
$ info gnuastro
If you couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users
and developers. For more information, please run:
$ info help-gnuastro
MakeCatalog options:
Input:
--clumpshdu=STR
Clump labels extension name or number.
-h, --hdu=STR/INT
Extension name or number of input data.
-l, --clumpsfile=STR
Dataset containing clump labels.
-s, --insky=STR/FLT
Input Sky value or dataset.
--skyhdu=STR
Sky image extension name or number.
--stdhdu=STR
Sky STD extension name or number.
--subtractsky
Subtract the Sky dataset from the values.
-t, --instd=STR/FLT
Sky standard deviation value or dataset.
-v, --valuesfile=STR
Values/brightness dataset.
--valueshdu=STR
Name or number of extension containing values.
--variance
STD input dataset is actually variance.
--zeropoint=FLT
Zeropoint magnitude of input dataset.
Tessellation (tile grid):
--checktiles
Tile IDs in an image, the size of input.
-F, --remainderfrac=FLT
Fraction of remainder to split last tile.
--interpmetric=INT
Interpolation metric (radial, manhattan).
-M, --numchannels=INT[,..] No. of channels in dim.s (FITS order).
--oneelempertile
Display 1 element/tile, not full input res.
-Z, --tilesize=INT[,INT]
Regular tile size on dim.s (FITS order).
Output:
-C, --clumpscat
Make a clumps catalog also.
-D, --dontdelete
Don't delete output if it exists.
--inbetweenints
Keep rows (integer ids) with no labels.
-K, --keepinputdir
Keep input directory for automatic output.
--noclumpsort
Don't sort the clumps catalog by ID.
-o, --output=STR
Output file name.
--sfmagarea=FLT
Surface brightness area (in arcseconds^2).
--sfmagnsigma=FLT
Surface brightness multiple of Sky STD.
--spectrum
Object spectrum for cube (3D) datasets.
--tableformat=STR
Table fmt: `fits-ascii', `fits-binary', `txt'.
Upper limit magnitude settings:
--checkuplim=INT[,INT] Check random distribution for one label.
-e, --envseed
Use GSL_RNG_SEED environment variable for seed.
--upmaskfile=STR
Mask image file name only for upper limit.
--upmaskhdu=STR
Mask image HDU only for upper limit.
--upnsigma=FLT
Multiple of sigma to define upperlimit.
--upnum=INT
Number of randomly positioned samples
--uprange=INT,INT
Range of random positions (pix) around target.
--upsigmaclip=FLT,FLT
Sigma multiple and, tolerance or number.
Identifier columns
-i, --ids
All IDs of objects and clumps.
--idinhostobj
ID of clump in host object.
-j, --hostobjid
ID of object hosting this clump.
--objid
Object label/ID.
Positional columns (pixel)
--clumpsgeox
Geometric center of all clumps in obj. (X).
--clumpsgeoy
Geometric center of all clumps in obj. (Y).
--clumpsgeoz
Geometric center of all clumps in obj. (Z).
--clumpsx
Flux.wht center of all clumps in obj. (X).
--clumpsy
Flux.wht center of all clumps in obj. (Y).
--clumpsz
Flux.wht center of all clumps in obj. (Z).
--geox Geometric center in first FITS axis.
--geoy Geometric center in second FITS axis.
--geoz Geometric center in third FITS axis.
--maxx Maximum first FITS axis position.
--maxy Maximum second FITS axis position.
--maxz Maximum third FITS axis position.
--minx Minimum first FITS axis position.
--miny Minimum second FITS axis position.
--minz Minimum third FITS axis position.
-x, --x
Flux weighted center in first FITS axis.
-y, --y
Flux weighted center in second FITS axis.
-z, --z
Flux weighted center in third FITS axis.
Positional columns (WCS)
--clumpsgeow1
Geometric center of all clumps in 1st WCS.
--clumpsgeow2
Geometric center of all clumps in 2nd WCS.
--clumpsgeow3
Geometric center of all clumps in 3rd WCS.
--clumpsw1
Flux.wht center of all clumps in 1st WCS.
--clumpsw2
Flux.wht center of all clumps in 2nd WCS.
--clumpsw3
Flux.wht center of all clumps in 3rd WCS.
-d, --dec
Flux weighted center declination.
--geow1
Geometric center in first WCS axis.
--geow2
Geometric center in second WCS axis.
--geow3
Geometric center in third WCS axis.
-r, --ra
Flux weighted center right ascension.
--w1 Flux weighted center in first WCS axis.
--w2 Flux weighted center in second WCS axis.
--w3 Flux weighted center in third WCS axis.
Brightness/magnitude related columns
-b, --brightness
Brightness (sum of pixel values).
--brightnesserr
Error (1-sigma) in measuring brightness.
--brightnessnoriver
Sky (not river) subtracted clump brightness.
--clumpbrightness
Brightness of clumps in an object.
--clumpsmagnitude
Magnitude of all clumps in object.
-G, --magnitudeerr
Magnitude error of objects or clumps.
--mean Mean of values in object/clump.
--median
Median of values in object/clump.
-m, --magnitude
Total magnitude of objects or clumps.
-n, --sn
Signal to noise ratio of objects or clumps.
--riverave
Average river value surrounding a clump.
--rivernum
Number of river pixels around a clump.
--sky Sky value (per pixel).
--std Sky standard deviation (per pixel).
--upperlimit
Upper-limit value, use other options to config.
-u, --upperlimitmag
Upper-limit mag. use other options to config.
--upperlimitonesigma
Upper-limit one sigma value.
--upperlimitquantile
Quantile in random distribution (max 1).
--upperlimitsigma
Place in random distribution (sigma multiple).
--upperlimitskew
(Mean-Median)/STD of random distribution.
Morphology/shape related columns
-a, --area
Number of non-blank valued pixels.
--areaxy
Projected area in first two dimensions.
-A, --semimajor
RMS along major axis (in pixels).
-B, --semiminor
RMS along minor axis (in pixels).
-c, --numclumps
Number of clumps in this object.
--clumpsarea
Non-blank area covered by clumps.
--geoarea
Area labled region (irrespective of value).
--geoareaxy
Projected geoarea in first two dimensions.
--geoaxisratio
Geometric axis ratio.
--geopositionangle
Geometric position angle.
--geosemimajor
RMS along major axis (ignoring value).
--geosemiminor
RMS along minor axis (ignoring value).
-p, --positionangle
Flux weighted position angle.
-Q, --axisratio
Flux weighted axis ratio.
--weightarea
Area used for value weighted positions.
Operating modes:
-?, --help
give this help list
--checkconfig
List all config files and variables read.
--cite BibTeX citation for this program.
--config=STR
Read configuration file STR immediately.
--lastconfig
Do not parse any more configuration files.
--minmapsize=INT
Minimum bytes in array to not use ram RAM.
-N, --numthreads=INT
Number of CPU threads to use.
--onlyversion=STR
Only run if the program version is STR.
-P, --printparams
Print parameter values to be used and abort.
-q, --quiet
Only report errors, remain quiet about steps.
--quietmmap
Don't print mmap'd file's name and size.
-S, --setdirconf
Set default values for this directory and abort.
--usage
give a short usage message
-U, --setusrconf
Set default values for this user and abort.
-V, --version
print program version
Mandatory or optional arguments to long options are also mandatory or optional for any corresponding
short options.
GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/
REPORTING BUGS
Report bugs to bug-gnuastro@gnu.org.
COPYRIGHT
Copyright © 2015-2019, Free Software Foundation, Inc. License GPLv3+: GNU General public license version
3 or later.
This is free software: you are free to change and redistribute it. There is NO WARRANTY, to the extent
permitted by law.
Written/developed by Mohammad Akhlaghi
SEE ALSO
The full documentation for MakeCatalog is maintained as a Texinfo manual. If the info and MakeCatalog
programs are properly installed at your site, the command
info MakeCatalog
should give you access to the complete manual.