reproject_and_coadd¶
-
reproject.mosaicking.reproject_and_coadd(input_data, output_projection, shape_out=None, input_weights=None, hdu_in=None, reproject_function=None, hdu_weights=None, combine_function='mean', match_background=False, background_reference=None, **kwargs)[source]¶ Given a set of input images, reproject and co-add these to a single final image.
This currently only works with 2-d images with celestial WCS.
Parameters: - input_data : iterable
One or more input datasets to include in the calculation of the final WCS. This should be an iterable containing one entry for each dataset, where a single dataset is one of:
- The name of a FITS file
- An
HDUListobject - An image HDU object such as a
PrimaryHDU,ImageHDU, orCompImageHDUinstance - A tuple where the first element is an
ndarrayand the second element is either aWCSor aHeaderobject
- output_projection :
WCSorHeader The output projection, which can be either a
WCSor aHeaderinstance.- shape_out : tuple, optional
If
output_projectionis aWCSinstance, the shape of the output data should be specified separately.- input_weights : iterable
If specified, this should be an iterable with the same length as
input_data, where each item is one of:- The name of a FITS file
- An
HDUListobject - An image HDU object such as a
PrimaryHDU,ImageHDU, orCompImageHDUinstance - An
ndarrayarray
- hdu_in : int or str, optional
If one or more items in
input_datais a FITS file or anHDUListinstance, specifies the HDU to use.- reproject_function : callable
The function to use for the reprojection
- combine_function : { ‘mean’, ‘sum’, ‘median’ }
The type of function to use for combining the values into the final image.
- match_background : bool
Whether to match the backgrounds of the images.
- background_reference :
Noneorint If
None, the background matching will make it so that the average of the corrections for all images is zero. If an integer, this specifies the index of the image to use as a reference.- kwargs
Keyword arguments to be passed to the reprojection function.