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Incorporating the addition of emission lines in the spectra using ProSpect features.
Additions needed include:
Working with both the gas and stellar information when in mode="spectral" - relevant gas particle/cell properties such as elemental abundances necessary to be included for each spaxel.
Assumed dust attenuation laws? Necessary to make clear that these are models and not produced in the underlying simulation. Likely to work with the models from ProSpect - i.e. Charlot and Fall model for birth cloud and screen dust attenuation and re-emission from MIR to FIR flux via the incorporation of the most recent Dale dust templates that model the heating of dust by a radiation field and AGN.
The text was updated successfully, but these errors were encountered:
Incorporating the addition of emission lines in the spectra using ProSpect features.
Additions needed include:
mode="spectral"
- relevant gas particle/cell properties such as elemental abundances necessary to be included for each spaxel.The text was updated successfully, but these errors were encountered: