sdapy.snerun.snobject.calc_colors¶
- snobject.calc_colors(xpred=None, index=0, returnv=False, **kwargs)¶
Calculate colors for two bands.
- Parameters
- xpredlist
colour phases, if None will use observing epochs of the color_bands
- color_bandslist
two bands of the colour
- color_interpstr
estimate flux with data epoch less than than tdbin, or interpolation from GP/fits
- returnvbool
if return the colors, or store them in the class
- bin_rangelist
for bin method, predict range
- gp_rangelist
for GP method, predict range
- fit_rangelist
for fit method, predict range
- 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
See also