CCDData¶
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class
ccdproc.CCDData(*args, **kwd)[source]¶ Bases:
astropy.nddata.NDDataArrayA class describing basic CCD data
The CCDData class is based on the NDData object and includes a data array, uncertainty frame, mask frame, meta data, units, and WCS information for a single CCD image.
Parameters: The actual data contained in this
CCDDataobject. Note that this will always be copies by reference , so you should make copy thedatabefore passing it in if that’s the desired behavior.uncertainty :
StdDevUncertaintyorndarray,optional Uncertainties on the data.
mask :
ndarray, optionalMask for the data, given as a boolean Numpy array with a shape matching that of the data. The values must be
Falsewhere the data is valid andTruewhen it is not (like Numpy masked arrays). Ifdatais a numpy masked array, providingmaskhere will causes the mask from the masked array to be ignored.flags :
ndarrayorFlagCollection, optionalFlags giving information about each pixel. These can be specified either as a Numpy array of any type with a shape matching that of the data, or as a
FlagCollectioninstance which has a shape matching that of the data.wcs :
WCSobject, optionalWCS-object containing the world coordinate system for the data.
meta :
dict-like object, optionalMetadata for this object. “Metadata” here means all information that is included with this object but not part of any other attribute of this particular object. e.g., creation date, unique identifier, simulation parameters, exposure time, telescope name, etc.
unit :
Unitinstance or str, optionalThe units of the data.
Raises: ValueError
If the
uncertaintyormaskinputs cannot be broadcast (e.g., match shape) ontodata.Notes
CCDDataobjects can be easily converted to a regular- Numpy array using
numpy.asarray
For example:
>>> from ccdproc import CCDData >>> import numpy as np >>> x = CCDData([1,2,3], unit='adu') >>> np.asarray(x) array([1, 2, 3])
This is useful, for example, when plotting a 2D image using matplotlib.
>>> from ccdproc import CCDData >>> from matplotlib import pyplot as plt >>> x = CCDData([[1,2,3], [4,5,6]], unit='adu') >>> plt.imshow(x)
Methods
read(*args, **kwargs) Classmethodto create an CCDData instance based on aFITSfile. This method usesfits_ccddata_reader()with the provided parameters.write(*args, **kwargs) Writes the contents of the CCDData instance into a new FITSfile. This method usesfits_ccddata_writer()with the provided parameters.Attributes Summary
datadtypeheadermetashapesizeuncertaintyunitwcsMethods Summary
add(other[, compare_wcs])copy()Return a copy of the CCDData object. divide(other[, compare_wcs])multiply(other[, compare_wcs])subtract(other[, compare_wcs])to_hdu([hdu_mask, hdu_uncertainty, hdu_flags])Creates an HDUList object from a CCDData object. Attributes Documentation
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data¶
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dtype¶
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header¶
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meta¶
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shape¶
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size¶
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uncertainty¶
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unit¶
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wcs¶
Methods Documentation
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to_hdu(hdu_mask=u'MASK', hdu_uncertainty=u'UNCERT', hdu_flags=None)[source]¶ Creates an HDUList object from a CCDData object.
Parameters: hdu_mask, hdu_uncertainty, hdu_flags : str or None, optional
If it is a string append this attribute to the HDUList as
ImageHDUwith the string as extension name. Flags are not supported at this time. IfNonethis attribute is not appended. Default is'MASK'for mask,'UNCERT'for uncertainty andNonefor flags.Returns: hdulist : astropy.io.fits.HDUList object
Raises: ValueError
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self.maskis set but not andarray. - If
self.uncertaintyis set but not aStdDevUncertainty. - If
self.uncertaintyis set but has another unit thenself.data.
NotImplementedError
Saving flags is not supported.
- If