ó ›ßÈ[c@ sadZddlmZyddlTddlmZWnek rSesT‚qTnXd„ZdS(sî .. _wcslib: http://www.atnf.csiro.au/people/mcalabre/WCS/wcslib/index.html .. _distortion paper: http://www.atnf.csiro.au/people/mcalabre/WCS/dcs_20040422.pdf .. _SIP: http://irsa.ipac.caltech.edu/data/SPITZER/docs/files/spitzer/shupeADASS.pdf .. _FITS WCS standard: https://fits.gsfc.nasa.gov/fits_wcs.html `astropy.wcs` contains utilities for managing World Coordinate System (WCS) transformations in FITS files. These transformations map the pixel locations in an image to their real-world units, such as their position on the sky sphere. It performs three separate classes of WCS transformations: - Core WCS, as defined in the `FITS WCS standard`_, based on Mark Calabretta's `wcslib`_. See `~astropy.wcs.Wcsprm`. - Simple Imaging Polynomial (`SIP`_) convention. See `~astropy.wcs.Sip`. - table lookup distortions as defined in WCS `distortion paper`_. See `~astropy.wcs.DistortionLookupTable`. Each of these transformations can be used independently or together in a standard pipeline. iÿÿÿÿ(tdivisioni(t*(tutilscC s+ddl}|jj|jjtƒdƒS(s7 Get the path to astropy.wcs's C header files. iÿÿÿÿNtinclude(tostpathtjointdirnamet__file__(R((s3lib/python2.7/site-packages/astropy/wcs/__init__.pyt get_include%s N( t__doc__t __future__RtwcstRt ImportErrort_ASTROPY_SETUP_R (((s3lib/python2.7/site-packages/astropy/wcs/__init__.pyts