B îq\ ã@sFdZddddgZd dd„Zddd„Zdd d„Zdd d„Zdd d„Zd S)zJ astropy.wcs-specific utilities for generating boilerplate in docstrings. ÚTWO_OR_MORE_ARGSÚRETURNSÚORIGINÚ RA_DEC_ORDERécCs | d¡}dd|}| |¡S)NÚ ú )ÚsplitÚjoin)ZcontentÚindentÚlines©r ú3lib/python3.7/site-packages/astropy/wcs/_docutil.pyÚ_fix s  rcCstd |¡|ƒS)Naçargs : 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. )rÚformat)Znaxisr r r r rscCstd |¡|ƒS)Nzresult : 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.)rr)Zout_typer r r r r#scCs td|ƒS)Nz¦ 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 r r r r*scCs td|ƒS)Nzü 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 r r r r4sN)r)r)r)r)r)Ú__doc__Ú__all__rrrrrr r r r Ús