sdapy.snerun.snobject.bb_colors¶

snobject.bb_colors(xpred=None, index=0, returnv=False, **kwargs)¶

Match or interpolate multiple band LCs, for blackbody (BB) construction.

Parameters

xpredlist: colour phases, if None will use observing epochs of the sed_bands
sed_bandslist: multiple bands of the BB
sed_ref_bandslist: reference filters been used to provide epochs as for bolometric LCs, e.g. give a list [‘g’,’r’], will create bolometric LCs with g and r epochs, or None on all epochs that had ever been observed.
sed_color_interpstr: estimate flux with data epoch less than than tdbin, or interpolation from GP/fits
tdbinfloat: threshold for binning
corr_mkwbool: if correct milky way extinction
corr_hostbool: if host galaxy extinction
indexint: if multiple models available, which of them to be used
quantilelist: use 50 percentile as mean, and 1 sigma (68%% -> 16%% - 84%%) as errors
clobberbool: Redo analysis
zpfloat: zeropoint to convert magnitude to flux. zp = 23.9 for micro Jansky to AB mag zp = 48.6 for ergs/s/cm2/Hz to AB mag e.g. mab = -2.5 * log10(fv[Jy]/3631) = -2.5 * log10(fv[mJy]) + 2.5*log10(3631*1e6)
snrtfloat: SNR threshold to distinguish detection/limit
returnvbool: if return the SED, or store them in the class