compute_sps_params¶
- grizli.fitting.compute_sps_params(full='j021820-051015_01276.full.fits', cosmology=FlatLambdaCDM(name='Planck15', H0=<Quantity 67.74 km / (Mpc s)>, Om0=0.3075, Tcmb0=<Quantity 2.7255 K>, Neff=3.046, m_nu=<Quantity [0., 0., 0.06] eV>, Ob0=0.0486))[source]¶
Compute stellar population parameters from a
GroupFitteroutput file.- Parameters
- fullstr,
HDUList Output from
GroupFitterwith the best-fit template coefficients. If a string, will be opened withastropy.io.fits.open. Default isj021820-051015_01276.full.fits.- cosmology
FLRW Cosmology object to compute luminosity distances.
- fullstr,
- Returns
- spsdict
Dictionary with the following keys:
Lv,MLv,MLv_rms,SFRv,SFRv_rms,templ. The first four areQuantityobjects with units of solar luminosity, solar mass per solar luminosity, solar mass per year, and solar mass per year, respectively. Thetemplkey is aSpectrumTemplateobject with the best-fit template.