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This is a version 2 challenge but flagging now since it will need considerable development.
In the future we will have grids that potentially have much higher dimensionality, with multiple photoionisation parameters. This posses a challenge because the grids could become very large, there will also be significant repetition. For example, the same incident spectra may exist multiple times.
I think this can be addressed with the following steps:
store the incident spectra with only the incident aces (e.g. age and metallicity). When extracting spectra only the incident axes would be used.
compress the nebular_continuum spectra using PCA, NNMF etc. In the context of PCA (probably not the best approach) the grid would contain the principle components and then the parameters at every (incident + photoionisation) grid point.
construct the linecont spectra from a LineCollection.
construct the nebular spectra from nebular_continuum and linecont.
calculate the transmission=transmitted/incident and compress. The rationale here is that the transmission should be relatively simple.
construct the transmitted spectra from the transmission and incident.
The text was updated successfully, but these errors were encountered:
This is a version 2 challenge but flagging now since it will need considerable development.
In the future we will have grids that potentially have much higher dimensionality, with multiple photoionisation parameters. This posses a challenge because the grids could become very large, there will also be significant repetition. For example, the same incident spectra may exist multiple times.
I think this can be addressed with the following steps:
incident
spectra with only the incident aces (e.g. age and metallicity). When extracting spectra only the incident axes would be used.nebular_continuum
spectra using PCA, NNMF etc. In the context of PCA (probably not the best approach) the grid would contain the principle components and then the parameters at every (incident + photoionisation) grid point.linecont
spectra from a LineCollection.nebular
spectra fromnebular_continuum
andlinecont
.transmission
=transmitted/incident
and compress. The rationale here is that the transmission should be relatively simple.transmitted
spectra from thetransmission
andincident
.The text was updated successfully, but these errors were encountered: