SpectralQuantity¶
- class astropy.coordinates.SpectralQuantity(value, unit=None, doppler_rest=None, doppler_convention=None, **kwargs)[source]¶
Bases:
SpecificTypeQuantity
One or more value(s) with spectral units.
The spectral units should be those for frequencies, wavelengths, energies, wavenumbers, or velocities (interpreted as Doppler velocities relative to a rest spectral value). The advantage of using this class over the regular
Quantity
class is that inSpectralQuantity
, theu.spectral
equivalency is enabled by default (allowing automatic conversion between spectral units), and a preferred Doppler rest value and convention can be stored for easy conversion to/from velocities.- Parameters:
- value
ndarray
orQuantity
orSpectralQuantity
Spectral axis data values.
- unitastropy:unit-like
Unit for the given data.
- doppler_rest
Quantity
[:ref: ‘speed’], optional The rest value to use for conversions from/to velocities
- doppler_convention
python:str
, optional The convention to use when converting the spectral data to/from velocities.
- value
Attributes Summary
The defined convention for conversions to/from velocity space.
The rest value of the spectrum used for transformations to/from velocity space.
Methods Summary
to
(unit[, equivalencies, doppler_rest, ...])Return a new
SpectralQuantity
object with the specified unit.to_value
([unit])The numerical value, possibly in a different unit.
Attributes Documentation
- doppler_convention¶
The defined convention for conversions to/from velocity space.
- Returns:
python:str
One of ‘optical’, ‘radio’, or ‘relativistic’ representing the equivalency used in the unit conversions.
- doppler_rest¶
The rest value of the spectrum used for transformations to/from velocity space.
- Returns:
Quantity
[:ref: ‘speed’]Rest value as an astropy
Quantity
object.
Methods Documentation
- to(unit, equivalencies=[], doppler_rest=None, doppler_convention=None)[source]¶
Return a new
SpectralQuantity
object with the specified unit.By default, the
spectral
equivalency will be enabled, as well as one of the Doppler equivalencies if converting to/from velocities.- Parameters:
- unitastropy:unit-like
An object that represents the unit to convert to. Must be an
UnitBase
object or a string parseable by theunits
package, and should be a spectral unit.- equivalencies
python:list
ofEquivalency
, optional A list of equivalence pairs to try if the units are not directly convertible (along with spectral). See Equivalencies. If not provided or
[]
, spectral equivalencies will be used. IfNone
, no equivalencies will be applied at all, not even any set globally or within a context.- doppler_rest
Quantity
[:ref: ‘speed’], optional The rest value used when converting to/from velocities. This will also be set at an attribute on the output
SpectralQuantity
.- doppler_convention{‘relativistic’, ‘optical’, ‘radio’}, optional
The Doppler convention used when converting to/from velocities. This will also be set at an attribute on the output
SpectralQuantity
.
- Returns:
SpectralQuantity
New spectral coordinate object with data converted to the new unit.
- to_value(unit=None, *args, **kwargs)[source]¶
The numerical value, possibly in a different unit.
- Parameters:
- unitastropy:unit-like, optional
The unit in which the value should be given. If not given or
None
, use the current unit.- equivalencies
python:list
ofpython:tuple
, optional A list of equivalence pairs to try if the units are not directly convertible (see Equivalencies). If not provided or
[]
, class default equivalencies will be used (none forQuantity
, but may be set for subclasses). IfNone
, no equivalencies will be applied at all, not even any set globally or within a context.
- Returns:
- value
ndarray
or scalar The value in the units specified. For arrays, this will be a view of the data if no unit conversion was necessary.
- value
See also
to
Get a new instance in a different unit.