Package pysynphot :: Module observationmode :: Class ObservationMode

Class ObservationMode

Instance Methods

__init__(self, obsmode, method='HSTGraphTable', graphtable=None, comptable=None)
x.__init__(...) initializes x; see x.__class__.__doc__ for signature source code

_getOpticalComponents(self, throughput_filenames)

source code

Sensitivity(self)
Calculate the sensitivity by combining the throughput curves with hc/lambda to convert erg/cm^2/sec/Angstrom to counts/sec.

source code

Throughput(self)
Throughput returns the TabularSpectralElement obtained by multiplying the SpectralElement components together.

source code

_multiplyThroughputs(self, index)

source code

ThermalSpectrum(self)

source code

Inherited from BaseObservationMode: GetFileNames, __len__, __str__, bandWave, showfiles

Inherited from BaseObservationMode (private): _computeBandwave, _computeQuadraticCoefficients, _getBandwaveFomFile, _getFileNames

Inherited from object: __delattr__, __getattribute__, __hash__, __new__, __reduce__, __reduce_ex__, __repr__, __setattr__

Properties

[hide private]

Inherited from object: __class__

Method Details

[hide private]

init(self, obsmode, method=`'HSTGraphTable'`, graphtable=None, comptable=None)
(Constructor)

source code

x.__init__(...) initializes x; see x.__class__.__doc__ for signature

Overrides: object.__init__: (inherited documentation)

Sensitivity(self)

source code

Calculate the sensitivity by combining the throughput curves with hc/lambda to convert erg/cm^2/sec/Angstrom to counts/sec. Multiplying this by the flux in erg/cm^2/sec/Angstrom will give counts/sec/Angstrom

Throughput(self)

source code

Throughput returns the TabularSpectralElement obtained by multiplying the SpectralElement components together. Unitless

Class ObservationMode

__init__(self, obsmode, method='HSTGraphTable', graphtable=None, comptable=None) (Constructor)

Sensitivity(self)

Throughput(self)

init(self, obsmode, method=`'HSTGraphTable'`, graphtable=None, comptable=None)
(Constructor)