Thomas Robitaille
Thomas Robitaille
Would it be helpful to keep track of all region classes? We can do that with a simple meta-class (I could add it)
PR #71 adds to_mask for some of the single regions, but in future we'll need to implement it on Compound regions. This will have varying degrees of difficulty depending on...
Currently, the ``.visual`` property is just a free-form dictionary which allows things such as: ``` region.visual['banana'] = 'apple' ``` We should make sure we validate the keys/values for this dictionary...
I am seeing a very strange issue. The following example tries to reproject a dataset with a GWCS to a slightly different GWCS: ```python import os import asdf from copy...
The main functions in reproject, such as ``reproject_interp``, accept ``parallel=`` and ``block_size=`` arguments which, if used, will leverage dask behind the scenes to split up the data into chunks and...
At the moment, we force cdelt[0] to be negative but this isn't true for e.g. solar data. We should avoid this!
This is an experiment for now but it allows: * N-dimensional reprojection/co-addition * ``combine_function='median'`` (not implemented here but trivial to do) * ``reproject_and_coadd`` to optionally return a dask array (``return_type='dask'``)...
This builds on https://github.com/astropy/reproject/pull/374 to add a possible mode where if we are dealing with arrays with extra/broadcasted dimensions, we can split up the input array into chunks along the...
Unfortunately enabling the limited Python API might not be easy yet because we use Cython and support for the limited API there is still experimental.
Currently when in parallel mode, if a user specifies a filename for the input file we load the data with astropy.io.fits, which even if memory mapped is then written out...