The final step of the calwebb_tso3 pipeline for spectroscopy data needs to produce an integrated ("white light") flux as a function of time. This will be done by simply integrating the extracted 1D flux spectrum over all wavelengths for all integrations within all exposures of a TSO. A new data product will be created that contains the light curve as a function of time.
hbushouse
commented
7 years ago
The final step of the calwebb_tso3 pipeline for spectroscopy data needs to produce an integrated ("white light") flux as a function of time. This will be done by simply integrating the extracted 1D flux spectrum over all wavelengths for all integrations within all exposures of a TSO. A new data product will be created that contains the light curve as a function of time.
This is a carryover of Trac ticket 372: https://aeon.stsci.edu/ssb/trac/jwst/ticket/372