Struct SEDlight

Defined in File SED.h

Struct Documentation

struct SEDlight

Structure with a light SED vector.

This structure is a light version of the class SED. It propose a light version to be used in fit

Public Functions

inline void push_sed(SED const &src, const array<double, 3> &colRFin)

Append the relevant attributes of a SED template to this light library

Parameters:

src – the SED template to append
colRFin – rest-frame colors of src, stored in colRF

Public Members

vector<object_type> nlib: object type (GAL/QSO/STAR) of each template

vector<int> index: index in the full SED library

vector<int> nummod: index in the initial list of rest-frame SEDs

vector<int> extlawId: index of the extinction law applied

vector<int> index_z0: index of the z=0 version of the template

vector<double> red: redshift

vector<double> chi2: best-fit chi2

vector<double> dm: normalization of the SED

vector<double> luv: monochromatic UV luminosity (see SED::luv)

vector<double> lopt: monochromatic optical luminosity (see SED::lopt)

vector<double> lnir: monochromatic NIR luminosity (see SED::lnir)

vector<double> mag0: z=0 reference-band magnitude (see SED::mag0)

vector<double> smag0: 10^(0.4*mag0): scale used by the log-free absolute-magnitude prior test in onesource::fit

vector<double> ebv: E(B-V) extinction value.

vector<double> lgage: log age (yr)

vector<double> lgmass: log stellar mass

vector<double> lgsfr: log SFR

vector<double> lgssfr: log specific SFR

vector<double> ltir: IR luminosity (see SED::ltir)

vector<array<double, 3>> colRF: rest-frame colors of each template