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The current set of LRG templates are just >1 Gyr-old simple stellar populations (SSPs) based on theoretical calculations by C. Conroy & collaborators. The current plan for hewing these templates more closely to data is to stack SEQUELS/LRG spectra and then to fit non-negative linear combinations of Charlie's SSPs to those spectra.
The text was updated successfully, but these errors were encountered:
The current set of LRG templates are just >1 Gyr-old simple stellar populations (SSPs) based on theoretical calculations by C. Conroy & collaborators. The current plan for hewing these templates more closely to data is to stack SEQUELS/LRG spectra and then to fit non-negative linear combinations of Charlie's SSPs to those spectra.
The text was updated successfully, but these errors were encountered: