.TH AN-FITSTOPNM "1" "July 2015" "0.56" "astrometry.net"
.SH NAME
an-fitstopnm \- Convert FITS images into ugly PNM images.
.SH SYNOPSIS
an\-fitstopnm \fB\-i\fR \fIinput-file\fR
.SH OPTIONS
.TP
\fB\-o\fR \fIfile\fR
Output file (default stdout)
.TP
\fB\-e\fR \fIext\fR
FITS extension number (default 0)
.TP
\fB\-p\fR \fIplane\fR
Image plane number (default 0)
.TP
\fB\-m\fR \fImargin\fR
Number of pixels to avoid at the image edges (default 0)
.TP
\fB\-O\fR
Do ordinal transform (default: map 25-95 percentile)
.TP
\fB\-L\fR \fIpercentile\fR
Set percentile that becomes black (default 25)
.TP
\fB\-H\fR \fIpercentile\fR
Set percentile that becomes white (default 95)
.TP
\fB\-I\fR
Invert black-on-white image
.TP
\fB\-X\fR \fImax\fR
Set the input value that will become white
.TP
\fB\-N\fR \fImin\fR
Set the input value that will become black
.TP
\fB\-x\fR
Set max to the observed maximum value
.TP
\fB\-n\fR
Set min to the observed minimum value
.TP
\fB\-r\fR
Same as \fB\-x\fR \fB\-n\fR: set min and max to observed data range.
.TP
\fB\-s\fR
Write 16-bit output
.TP
\fB\-v\fR
Verbose
.TP
\fB\-M\fR
Compute & print median value
.SH AUTHOR
The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and
Dustin Lang (CMU).
.SH SEE ALSO
http://astrometry.net