QSOSED_L2500#
Name#
QSOSED_L2500
Purpose#
Generates the qsosed \(L_{2500}\) (monochromatic luminosity at 2500 Angstroms) corresponding to given values of \(M\) and \(\log(\dot{M})\) using the models from Kubota & Done (2018).
Calling Sequence#
L2500 = qsosed_L2500(xray_models, agn_mass, agn_logmdot [, /error_check])
Inputs#
xray_models
structureA structure containing the spectra, counts, and X-ray model parameters. (See
xrb_xagn_models.pro
for details and contents.)agn_mass
int, float, or double array(Nmodels)Supermassive black hole mass \([M_\odot]\).
agn_logmdot
int, float, or double array(Nmodels)Log10 of SMBH accretion rate, normalized by the Eddington rate.
Optional Input#
error_check
flagIf set, all inputs are checked for errors. Otherwise, all inputs are assumed to be of correct format.
Output#
L2500
double array(Nmodels)The interpolated rest-frame 2500 Angstrom monochromatic luminosity of shifted to the observed frame \([L_\odot\ {\rm Hz}^{-1}]\).
Reference#
Modification History#
2022/04/18: Created (Erik B. Monson)
2022/06/10: Added error handling (Keith Doore)
2022/06/10: Added
error_check
keyword to do error handling (Keith Doore)2022/06/10: Made
mass
andlogmdot
required inputs (Keith Doore)