sourcefinder.accessors.fitsimageblob
====================================

.. py:module:: sourcefinder.accessors.fitsimageblob


Attributes
----------

.. autoapisummary::

   sourcefinder.accessors.fitsimageblob.logger


Classes
-------

.. autoapisummary::

   sourcefinder.accessors.fitsimageblob.FitsImageBlob


Module Contents
---------------

.. py:class:: FitsImageBlob(hdulist, plane=None, beam=None, hdu_index=0)

   Bases: :py:obj:`sourcefinder.accessors.fitsimage.FitsImage`


   
   A FITS image blob. Same as ``sourcefinder.accessors.fitsimage.FitsImage``
   but constructed from an in-memory FITS file, not a FITS file on disk.


   :Parameters:

       **hdulist** : astropy.io.fits.HDUList
           The HDU list representing the in-memory FITS file.

       **plane** : int, default: None
           If the data is a datacube, specifies which plane to use.

       **beam** : tuple, default: None
           Beam parameters in degrees, in the form (bmaj, bmin, bpa). If not 
           supplied, the method will attempt to read these from the header.

       **hdu_index** : int, default: 0
           The index of the HDU to use from the HDU list.














   ..
       !! processed by numpydoc !!

   .. py:method:: _get_header(*args)

      
      Retrieve the header from the specified HDU.


      :Parameters:

          **\*args** : tuple
              Positional arguments where:
              
              - args[0] is the HDU list (astropy.io.fits.HDUList).
              - args[1] is the index of the HDU to use.



      :Returns:

          astropy.io.fits.Header
              The header of the specified HDU.











      ..
          !! processed by numpydoc !!


   .. py:method:: read_data(*args)

      
      Read and process the data from the specified HDU.


      :Parameters:

          **\*args** : tuple
              Positional arguments where:
              
              - args[0] is the HDU list (astropy.io.fits.HDUList).
              - args[1] is the index of the HDU to use.
              - args[2] is the plane index (int) if the data is a datacube.



      :Returns:

          numpy.ndarray
              The processed 2D data array. Processing here means remove axes of
              length 1, select the plane index from the datacube if needed, and
              transpose.











      ..
          !! processed by numpydoc !!


   .. py:attribute:: data


   .. py:attribute:: header


   .. py:attribute:: pixelsize


   .. py:attribute:: url
      :value: 'AARTFAAC streaming image'



   .. py:attribute:: wcs


.. py:data:: logger