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Sample populations using SkyPy #17
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This module, along with an SED library, is necessary to adapt a real galaxy catalog, e.g. COSMOS, to the desired target bandwidth. |
Hi @jiwoncpark Will the skypy libraries work for you? Having it integrated/compatible with skypy might be good in the long run as there is heavy development and wide use of this case in the project. |
Hi @sibirrer, awesome, thanks! I do want to maximize the use of well-validated modules from SkyPy and GalSim. This is a good early point to refactor Baobab to wrap more heavily around SkyPy. The workflow could then be:
Prescription for how to do the K-correction (source/target redshifts/bands, luminosity) would be propagated from 1 onto 2 and 3. |
This sounds excellent! |
Agreed that all these efforts can complement one another and converge at some point! I'm looking forward to chatting soon. Referencing Issue #56, which corresponds to Step 4. As mentioned there, my intermediate goal is to (1) describe LSST-like populations at the mag/size/color level, and (2) generate the corresponding images AND/OR query real images and adapt them to LSST specs (similar to the work by @swagnercarena @JelleAalbers and Elise). |
Class
KCorrector
accepts the SED, dust, and input/output filter throughputs and numerically integrates to get the K-corrected apparent magnitudeThe text was updated successfully, but these errors were encountered: