1WCS-PV2SIP(1)                   astrometry.net                   WCS-PV2SIP(1)
2
3
4

NAME

6       wcs-pv2sip - Convert TPV WCS headers to SIP distortion headers
7

SYNOPSIS

9       wcs-pv2sip [options] input-wcs output-wcs
10

OPTIONS

12       -o order
13              SIP polynomial order to fit (default: 5)
14
15       -e ext FITS HDU number to read WCS from (default 0 = primary)
16
17       -S     Do NOT do the wcs_shift thing
18
19       -s     Treat input as Scamp .head file
20
21       -t     Override the CTYPE* cards in the WCS header, and assume they are
22              TAN.
23
24       -v     +verboseness
25
26       -W int Set the IMAGEW in the output file
27
28       -H int Set the IMAGEH in the output file
29
30       -x num x-low (default: 1)
31
32       -y num y-low (default: 1)
33
34       -X num x-high (default: image width)
35
36       -Y num y-high (default: image width)
37
38       -a size
39              Set the pixel values used to compute the distortion  polynomials
40              with (default: closest to 100 yielding whole number of steps)
41

AUTHOR

43       The  Astrometry.net  team.  Principal  investigators  are David W. Hogg
44       (NYU) and Dustin Lang (CMU).
45

SEE ALSO

47       http://astrometry.net
48
49
50
510.56                               July 2015                     WCS-PV2SIP(1)
Impressum