synthpop.modules.extinction.hosek2018
Extinction law from Hosek et al (2018), representative of highly reddened
regions like young star clusters and the Galactic center.
Valid from 0.8 to 2.2 microns.
Source DOI: 10.3847/1538-4357/aaabbb
Code also available at https://github.com/mwhosek/extlaw_H18
Classes
Hosek2018
|
Extinction law from Hosek et al. (2018) |
Module Contents
-
class synthpop.modules.extinction.hosek2018.Hosek2018(**kwargs)
Bases: synthpop.modules.extinction._extinction.ExtinctionLaw
Extinction law from Hosek et al. (2018)
-
extinction_law_name = 'Hosek2018'
-
law_ref_wavelength = 2.14
-
min_wavelength = 0.8
-
max_wavelength = 2.2
-
Alambda_Aref(eff_wavelength: float) → float
Given an effective wavelength lambda_eff, calculate the relative extinction A_lambda/A_V
Parameters
- eff_wavelengthfloat
Effective Wavelength of the filter for which the extinction should be determined.
in micrometer