σ ›ίΘ[c@`szdZddlmZmZmZmZddddgZdd„Zdd„Zdd „Z dd „Z dd „Z d S( uJ astropy.wcs-specific utilities for generating boilerplate in docstrings. i(tabsolute_importtdivisiontprint_functiontunicode_literalsuTWO_OR_MORE_ARGSuRETURNSuORIGINu RA_DEC_ORDERcC`s*|jdƒ}dd|}|j|ƒS(Nu u (tsplittjoin(tcontenttindenttlines((s3lib/python2.7/site-packages/astropy/wcs/_docutil.pyt_fix scC`stdj|ƒ|ƒS(Nuηargs : flexible There are two accepted forms for the positional arguments: - 2 arguments: An *N* x *{0}* array of coordinates, and an *origin*. - more than 2 arguments: An array for each axis, followed by an *origin*. These arrays must be broadcastable to one another. Here, *origin* is the coordinate in the upper left corner of the image. In FITS and Fortran standards, this is 1. In Numpy and C standards this is 0. (R tformat(tnaxisR((s3lib/python2.7/site-packages/astropy/wcs/_docutil.pytTWO_OR_MORE_ARGSscC`stdj|ƒ|ƒS(Nuresult : array Returns the {0}. If the input was a single array and origin, a single array is returned, otherwise a tuple of arrays is returned.(R R (tout_typeR((s3lib/python2.7/site-packages/astropy/wcs/_docutil.pytRETURNS$scC`s td|ƒS(Nu¦ origin : int Specifies the origin of pixel values. The Fortran and FITS standards use an origin of 1. Numpy and C use array indexing with origin at 0. (R (R((s3lib/python2.7/site-packages/astropy/wcs/_docutil.pytORIGIN+scC`s td|ƒS(Nuό ra_dec_order : bool, optional When `True` will ensure that world coordinates are always given and returned in as (*ra*, *dec*) pairs, regardless of the order of the axes specified by the in the ``CTYPE`` keywords. Default is `False`. (R (R((s3lib/python2.7/site-packages/astropy/wcs/_docutil.pyt RA_DEC_ORDER5sN( t__doc__t __future__RRRRt__all__R R RRR(((s3lib/python2.7/site-packages/astropy/wcs/_docutil.pyts"