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This repository has been archived by the owner on Feb 27, 2023. It is now read-only.
The color evolution of the CMFGEN models are very similar for phases near peak B-band magnitude. To understand our ability to constrain the models in color space, we should plot the predicted SNR ratio of LSST as a function of phase and redshift (i.e., A 2d plot where SNR is a third, color axis).
This plot will involve combining information from the single visit quoted depth for LSST and a supernova model (likely Salt2).
The text was updated successfully, but these errors were encountered:
The color evolution of the CMFGEN models are very similar for phases near peak B-band magnitude. To understand our ability to constrain the models in color space, we should plot the predicted SNR ratio of LSST as a function of phase and redshift (i.e., A 2d plot where SNR is a third, color axis).
This plot will involve combining information from the single visit quoted depth for LSST and a supernova model (likely Salt2).
The text was updated successfully, but these errors were encountered: