def get_equivalencies():
"""
Return a list of example equivalencies for testing serialization.
"""
return [
eq.plate_scale(.3 * u.deg / u.mm),
eq.pixel_scale(.5 * u.deg / u.pix),
eq.spectral_density(350 * u.nm, factor=2),
eq.spectral_density(350 * u.nm),
eq.spectral(),
eq.brightness_temperature(500 * u.GHz),
eq.brightness_temperature(500 * u.GHz, beam_area=23 * u.sr),
eq.with_H0(),
eq.temperature_energy(),
eq.temperature(),
eq.thermodynamic_temperature(300 * u.Hz),
eq.thermodynamic_temperature(140 * u.GHz, Planck15.Tcmb0),
eq.beam_angular_area(3 * u.sr),
eq.mass_energy(),
eq.molar_mass_amu(),
eq.doppler_relativistic(2 * u.m),
eq.doppler_optical(2 * u.nm),
eq.doppler_radio(2 * u.Hz),
eq.parallax(),
eq.logarithmic(),
eq.dimensionless_angles(),
eq.spectral() + eq.temperature(),
(eq.spectral_density(35 * u.nm) +
eq.brightness_temperature(5 * u.Hz, beam_area=2 * u.sr)),
(eq.spectral() + eq.spectral_density(35 * u.nm) +
eq.brightness_temperature(5 * u.Hz, beam_area=2 * u.sr))
]
def to_flux(self, unit, equivalencies=None, suppress_conversion=False):
"""
Converts the flux data to the specified unit.
Parameters
----------
unit : str or `~astropy.units.Unit`
The unit to conver the flux array to.
equivalencies : list of equivalencies
Custom equivalencies to apply to conversions.
Set to spectral_density by default.
suppress_conversion : bool
Set to true if updating the unit without
converting data values.
Returns
-------
`~astropy.units.Quantity`
The converted flux array.
"""
if not suppress_conversion:
if equivalencies is None:
equivalencies = eq.spectral_density(self.spectral_axis)
new_data = self.flux.to(
unit, equivalencies=equivalencies)
self._data = new_data.value
self._unit = new_data.unit
else:
self._unit = u.Unit(unit)
return self.flux
def to_flux(self, unit, equivalencies=None, suppress_conversion=False):
"""
Converts the flux data to the specified unit.
Parameters
----------
unit : str or `~astropy.units.Unit`
The unit to conver the flux array to.
equivalencies : list of equivalencies
Custom equivalencies to apply to conversions.
Set to spectral_density by default.
suppress_conversion : bool
Set to true if updating the unit without
converting data values.
Returns
-------
`~astropy.units.Quantity`
The converted flux array.
"""
if not suppress_conversion:
if equivalencies is None:
equivalencies = eq.spectral_density(self.spectral_axis)
new_data = self.flux.to(
unit, equivalencies=equivalencies)
self._data = new_data.value
self._unit = new_data.unit
else:
self._unit = u.Unit(unit)
return self.flux
def to_flux(self, unit):
"""
Converts the flux data to the specified unit.
Parameters
----------
unit : str or ~`astropy.units.Unit`
The unit to conver the flux array to.
Returns
-------
~`astropy.units.Quantity`
The converted flux array.
"""
new_data = self.flux.to(
unit, equivalencies=eq.spectral_density(self.spectral_axis))
self._data = new_data.value
self._unit = new_data.unit
return self.flux
def new_flux_unit(self,
unit,
equivalencies=None,
suppress_conversion=False):
"""
Converts the flux data to the specified unit. This is an in-place
change to the object.
Parameters
----------
unit : str or `~astropy.units.Unit`
The unit to convert the flux array to.
equivalencies : list of equivalencies
Custom equivalencies to apply to conversions.
Set to spectral_density by default.
suppress_conversion : bool
Set to true if updating the unit without
converting data values.
Returns
-------
`~specutils.Spectrum1D`
A new spectrum with the converted flux array
"""
new_spec = deepcopy(self)
if not suppress_conversion:
if equivalencies is None:
equivalencies = eq.spectral_density(self.spectral_axis)
new_data = self.flux.to(unit, equivalencies=equivalencies)
new_spec._data = new_data.value
new_spec._unit = new_data.unit
else:
new_spec._unit = u.Unit(unit)
return new_spec
def to_flux(self, unit):
"""
Converts the flux data to the specified unit.
Parameters
----------
unit : str or ~`astropy.units.Unit`
The unit to conver the flux array to.
Returns
-------
~`astropy.units.Quantity`
The converted flux array.
"""
new_data = self.flux.to(unit,
equivalencies=eq.spectral_density(
self.spectral_axis))
self._data = new_data.value
self._unit = new_data.unit
return self.flux
def new_flux_unit(self, unit, equivalencies=None, suppress_conversion=False):
"""
Converts the flux data to the specified unit. This is an in-place
change to the object.
Parameters
----------
unit : str or `~astropy.units.Unit`
The unit to conver the flux array to.
equivalencies : list of equivalencies
Custom equivalencies to apply to conversions.
Set to spectral_density by default.
suppress_conversion : bool
Set to true if updating the unit without
converting data values.
Returns
-------
`~specutils.Spectrum1D`
A new spectrum with the converted flux array
"""
new_spec = deepcopy(self)
if not suppress_conversion:
if equivalencies is None:
equivalencies = eq.spectral_density(self.spectral_axis)
new_data = self.flux.to(
unit, equivalencies=equivalencies)
new_spec._data = new_data.value
new_spec._unit = new_data.unit
else:
new_spec._unit = u.Unit(unit)
return new_spec
