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calib_mag_zp_array=np.array([result.mag_zpornp.nanforresultinphotopolresult_Lifresult.astrosource.srctype==SRCTYPES.CALIBRATOR]) # else it fills with None also and the dtype becomes object
Might be interesting to use sigma clipping by default, it will make results more resilant to image defects and possibly bad calibrators.
The text was updated successfully, but these errors were encountered:
iop4/iop4lib/instruments/instrument.py
Line 595 in d8dfafa
Might be interesting to use sigma clipping by default, it will make results more resilant to image defects and possibly bad calibrators.
The text was updated successfully, but these errors were encountered: