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We are currently using the COSMOS example para file which is a significantly different regime to LSST. We need to develop a setup that is optimised for LSST.
Shall we remove emission lines?
Given the smaller number of bands can an n(z) prior be useful?
How should we optimise the template sets, extinction laws, and other parameters?
The text was updated successfully, but these errors were encountered:
We are currently using the COSMOS example para file which is a significantly different regime to LSST. We need to develop a setup that is optimised for LSST.
Shall we remove emission lines?
Given the smaller number of bands can an n(z) prior be useful?
How should we optimise the template sets, extinction laws, and other parameters?
The text was updated successfully, but these errors were encountered: