ModelData¶
- class measure_extinction.modeldata.ModelData(modelfiles, path='./', band_names=None, spectra_names=['BAND', 'STIS'])[source]¶
Bases:
objectProvide stellar atmosphere model “observed” data given input stellar, gas, and dust extinction parameters.
- Parameters:
- modelfiles: string array
set of model files to use
- pathstring, optional
path for model files
- band_namesstring array, optional
bands to use default = [‘U’, ‘B’, ‘V’, ‘J’, ‘H’, ‘K’]
- spectra_namesstring array, optional
origin of the spectra to use default = [‘STIS’]
- Attributes:
- n_modelsint
number of stellar atmosphere models
- model_filesstring array
filenames for the models
- tempsfloat array
log10(effective temperatures)
- gravsfloat array
log10(surface gravities)
- metsfloat array
log10(metallicities)
- vturbsfloat array
microturbulance values [km/s]
- n_bandsint
number of photometric bands
- band_namesstring array
names of the photometric bands
- n_spectraint
number of different types of spectra
- spectra_namesstring array
identifications for the spectra data (includes band data)
- wavesn_spectra dict
wavelengths for the spectra
- fluxesn_spectra dict
fluxes in the bands
- flux_uncsn_spectra list
flux uncertainties in the bands
Methods Summary
SED_to_StarData(sed)Convert the model created SED into a StarData object.
Methods Documentation