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astrofrog committed Sep 28, 2018
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status: Accepted

*Note: this APE14 was origially accepted on 2018-Feb-28, but due to issues with
implementation was significanly revised on 2018-May-23 and is under new review*
*Note: this APE14 was originally accepted on 2018-Feb-28, but due to issues with
implementation was significantly revised on 2018-May-23 and is under new review*

Abstract
--------
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We do not mandate a specific order for the world coordinates. While it might be
tempting to assume the 'same' order as for pixel coordinates, this only makes
sense for simple cases (for example an image of the sky where ra/dec are roughly
lined up with x/y). In a generalized WCS system, such a correspondance does not
lined up with x/y). In a generalized WCS system, such a correspondence does not
exist. As an example, consider an equatorial coordinate system rotated 45
degrees from the pixel coordinates. Such a system could be represented by the
following::
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and there is no 'right' order.
We note that the API we present here makes it easy to create a WCS with
reorederd world coordinates - this would involve changing the order of
reordered world coordinates - this would involve changing the order of
``world_axis_physical_types``, ``world_axis_units``, and
``world_axis_object_components``, changing the order of
``axis_correlation_matrix`` along the first dimension, and changing the order
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Additionally, for ``world_axis_physical_types``, an alternative was considered
of adopting a much more general set of terms vs UCD1+ such as ``"celestial"``,
``"spectral"``, etc. and just coming up with the list in this APE (possibly
using terms that approxmiately align with the STC standard). But it was decided
using terms that approximately align with the STC standard). But it was decided
that adopting the VO UCD1+ would be best because it would not lead to Astropy
needing to maintain a separate "standard" of terminology where one already
exists.
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