CCDData¶

class astropy.nddata.CCDData(*args, **kwd)[source]¶

Bases: astropy.nddata.NDDataArray

A class describing basic CCD data.

The CCDData class is based on the NDData object and includes a data array, uncertainty frame, mask frame, flag frame, meta data, units, and WCS information for a single CCD image.

Parameters

dataCCDData-like or numpy.ndarray-like: The actual data contained in this CCDData object. Note that the data will always be saved by reference, so you should make a copy of the data before passing it in if that’s the desired behavior.
uncertaintyStdDevUncertainty, VarianceUncertainty, InverseVariance, numpy.ndarray or None, optional: Uncertainties on the data. If the uncertainty is a numpy.ndarray, it it assumed to be, and stored as, a StdDevUncertainty. Default is None.
masknumpy.ndarray or None, optional: Mask for the data, given as a boolean Numpy array with a shape matching that of the data. The values must be False where the data is valid and True when it is not (like Numpy masked arrays). If data is a numpy masked array, providing mask here will causes the mask from the masked array to be ignored. Default is None.
flagsnumpy.ndarray or FlagCollection or None, optional: Flags 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 FlagCollection instance which has a shape matching that of the data. Default is None.
wcsWCS or None, optional: WCS-object containing the world coordinate system for the data. Default is None.
metadict-like object or None, optional: Metadata 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.
unitUnit or str, optional: The units of the data. Default is None.

Warning

If the unit is None or not otherwise specified it will raise a ValueError

Raises

ValueError: If the uncertainty or mask inputs cannot be broadcast (e.g., match shape) onto data.

Notes

CCDData objects can be easily converted to a regular: Numpy array using numpy.asarray.

For example:

>>> from astropy.nddata 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 astropy.nddata import CCDData
>>> from matplotlib import pyplot as plt   
>>> x = CCDData([[1,2,3], [4,5,6]], unit='adu')
>>> plt.imshow(x)   

Attributes

known_invalid_fits_unit_strings: A dictionary that maps commonly-used fits unit name strings that are technically invalid to the correct valid unit type (or unit string). This is primarily for variant names like “ELECTRONS/S” which are not formally valid, but are unambiguous and frequently enough encountered that it is convenient to map them to the correct unit.

Methods

*read(args, kwargs)	`Classmethod` to create an CCDData instance based on a `FITS` file. This method uses `fits_ccddata_reader()` with the provided parameters.
*write(args, kwargs)	Writes the contents of the CCDData instance into a new `FITS` file. This method uses `fits_ccddata_writer()` with the provided parameters.

Attributes Summary

`data`	`ndarray`-like : The stored dataset.
`header`
`known_invalid_fits_unit_strings`
`uncertainty`	any type : Uncertainty in the dataset, if any.
`unit`	`Unit` : Unit for the dataset, if any.
`wcs`	any type : A world coordinate system (WCS) for the dataset, if any.

Methods Summary

`add`(operand[, operand2])	See `astropy.nddata.NDArithmeticMixin.add`.
`copy`()	Return a copy of the CCDData object.
`divide`(operand[, operand2])	See `astropy.nddata.NDArithmeticMixin.divide`.
`multiply`(operand[, operand2])	See `astropy.nddata.NDArithmeticMixin.multiply`.
`subtract`(operand[, operand2])	See `astropy.nddata.NDArithmeticMixin.subtract`.
`to_hdu`([hdu_mask, hdu_uncertainty, …])	Creates an HDUList object from a CCDData object.

Attributes Documentation

data¶

header¶

known_invalid_fits_unit_strings = {'ELECTRONS': Unit("electron"), 'ELECTRONS/S': Unit("electron / s"), 'electrons': Unit("electron")}¶

uncertainty¶

unit¶

wcs¶

Methods Documentation

classmethod add(operand, operand2=None, **kwargs)¶: See astropy.nddata.NDArithmeticMixin.add.

copy()[source]¶: Return a copy of the CCDData object.

classmethod divide(operand, operand2=None, **kwargs)¶: See astropy.nddata.NDArithmeticMixin.divide.

classmethod multiply(operand, operand2=None, **kwargs)¶: See astropy.nddata.NDArithmeticMixin.multiply.

classmethod subtract(operand, operand2=None, **kwargs)¶: See astropy.nddata.NDArithmeticMixin.subtract.

to_hdu(hdu_mask='MASK', hdu_uncertainty='UNCERT', hdu_flags=None, wcs_relax=True, key_uncertainty_type='UTYPE')[source]¶

Creates an HDUList object from a CCDData object.

Parameters

hdu_mask, hdu_uncertainty, hdu_flagsstr or None, optional: If it is a string append this attribute to the HDUList as ImageHDU with the string as extension name. Flags are not supported at this time. If None this attribute is not appended. Default is 'MASK' for mask, 'UNCERT' for uncertainty and None for flags.
wcs_relaxbool: Value of the relax parameter to use in converting the WCS to a FITS header using to_header. The common CTYPE RA---TAN-SIP and DEC--TAN-SIP requires relax=True for the -SIP part of the CTYPE to be preserved.
key_uncertainty_typestr, optional: The header key name for the class name of the uncertainty (if any) that is used to store the uncertainty type in the uncertainty hdu. Default is UTYPE.

New in version 3.1.

Returns

hdulistHDUList

Raises

ValueError

If self.mask is set but not a numpy.ndarray.
If self.uncertainty is set but not a astropy uncertainty type.
If self.uncertainty is set but has another unit then self.data.

NotImplementedError

Saving flags is not supported.

Navigation

CCDData¶