sdapy.snerun.snobject._to_luminosity¶
- snobject._to_luminosity(m, f, em=None, **kwargs)¶
Convert magnitude to luminosity.
- Parameters
- mfloat
apparent (AB) magnitude. For UV/NIR, if input is AB, set
ab2vegaTrue, otherwise leave it False.- emfloat
apparent magnitude error
- fstr
filter
- ab2vegabool
set it True if input UV/IR data in AB, if they’re vega, set to False
- do_kcorrbool
K corrected the photometry or spectra
- Returns
- fluxfloat
flux, unit in erg/s/A
- dfluxfloat
flux error, unit in erg/s/A
- wfloat
central wavelength, unit in A
- bandwidthfloat
band width, unit in A