As a validation step for the data we are using, the published CSP photometry should be compared against the integrated flux from the spectroscopic observations. Steps for this include:
Pick a spectrum and photometric band-pass
Select the spectroscopic flux values in that band-pass
Integrate the observed flux times the band-pass transmission
Fit the light curve (most likely with a Gaussian regression for consistency)
Compare (tabulate) the fitted photometric value with the integrated flux value
Repeat for each spectrum / bandpass combo
This issue should culminate with a table having columns similar to obj_id, time, flux_val, phot_val.
We can use the DR1 data until DR2 is ported to SNData.
As a validation step for the data we are using, the published CSP photometry should be compared against the integrated flux from the spectroscopic observations. Steps for this include:
This issue should culminate with a table having columns similar to
obj_id,time,flux_val,phot_val.We can use the DR1 data until DR2 is ported to SNData.