.\" DO NOT MODIFY THIS FILE!  It was generated by help2man 1.49.3.
.TH BINCAT "1" "February 2024" "bincat EB_SOURCE" "User Commands"
.SH NAME
bincat \- AME
.SH SYNOPSIS
.B [-v][-a
\fI\,degrees\/\fR][\fI\,-p scale\/\fR][\fI\,-b ra dec\/\fR][\fI\,-j ra dec\/\fR][\fI\,-s nx ny\/\fR] \fI\,filename\/\fR
.SH DESCRIPTION
Bin catalog into a FITS image
.IP
[\-x x y] [\-c catname] file.fits ...
.HP
\fB\-a\fR ang: initial rotation angle in degrees (default 0)
.HP
\fB\-b\fR ra dec: initial center in B1950 (FK4) RA and Dec
.HP
\fB\-c\fR name: name of source catalog to bin
.HP
\fB\-d\fR: set CDELTn, CROTAn instead of CD matrix
.HP
\fB\-f\fR num: Set flux scaling factor (number if 0)
.HP
\fB\-g\fR long lat: initial center in Galactic longitude and latitude
.HP
\fB\-j\fR ra dec: initial center in J2000 (FK5) RA and Dec
.HP
\fB\-mx\fR mag1[,mag2]: Magnitude #x limit(s) (only one set allowed, default none)
.HP
\fB\-o\fR num: output pixel size in bits (FITS BITPIX, default=0)
.HP
\fB\-p\fR num: initial plate scale in arcsec per pixel (default 0)
.HP
\fB\-s\fR num num: size of image in x and y pixels (default 100x100)
.HP
\fB\-t\fR proj: set FITS CTYPE projection (default TAN)
.HP
\fB\-v\fR: verbose
.HP
\fB\-w\fR file: read WCS information from this FITS file
.HP
\fB\-x\fR x y: X and Y coordinates of reference pixel (default is center)
.HP
\fB\-z\fR: use AIPS classic projections instead of WCSLIB