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from .angles import Angle | |
from .. import units as u | |
import starlink.Ast as Ast | |
__all__ = [ 'SkyPosition', 'ICRSPosition', 'AZELPosition', | |
'ECLIPTICPosition', 'FK4Position', 'FK4_NO_EPosition', | |
'FK5Position', 'GALACTICPosition', 'GEOCENTRICPosition', | |
'HELIOECLIPTICPosition', 'J2000Position', | |
'SUPERGALACTICPosition', 'UNKNOWNPosition' ] |
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#!/bin/env python | |
# Rotates a simple 2D FITS image. If <xcen> and <ycen> are specified, | |
# the output image is the same size as the input image. Otherwise, | |
# the output image is the smallest that will hold all the rotated input | |
# data. | |
# Usage: | |
# rotate_wcs.py <infile> <outfile> <rotation> [<xcen> <ycen>] | |
# |
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#!/bin/env python | |
# Moves a simple 2D FITS image in X and Y. The output image is the same size as | |
# the input image. | |
# Usage: | |
# move_wcs.py <infile> <outfile> <xshift> <yshift> | |
# | |
# <infile> = Input fits file | |
# <outfile> = Output fits file |
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#!/bin/env python | |
# Re-projects a 2D FITS image so that it is aligned pixel-for-pixel with | |
# another reference FITS image. | |
# Usage: | |
# wcsalign.py <infile> <reffile> <outfile> | |
# | |
# <infile> = Input fits file | |
# <reffile> = Reference fits file |
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#!/usr/bin/env python | |
import starlink.Ast as Ast | |
# Create a text file containing an STC-S phrase. | |
with open("stcs1","w") as f: | |
f.write(''' | |
Union ICRS TOPOCENTER ( | |
Circle 180 10 20 | |
Circle 190 10 20 |