sdapy.snerun.snobject._get_fp_atlas

snobject._get_fp_atlas(f, binned=False, **kwargs)

(static) parse local ATLAS forced (binned or not binned) photometric data to snobject.lc

Parameters

fstr

ATLAS file name

binnedbool

if file is binned data or not

zpfloat

zeropoint to convert flux to magnitude. 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

snobject.add_lc, snobject.add_mag