Comments (3)
I'm not sure I understand how to implement what is being suggested here.
For the distance prior in the megabeast, it is something that will effect all the stars, not just specific parts of the HR diagram.
But plan is to set up the fitting to be able to limit it (if desired) to specific HR diagram region (see #43). Does this address this point?
from megabeast.
Perhaps my comment is off-base for how MegaBEAST will do things.
If I were to measure a distance from a CMD, I could fit, for example, the TRGB or the Horizontal Branch. Each of these has its own calibration. Fitting each individually and applying the calibrations can result in slightly different answers. Thus, it is sometimes useful to consider these distances determinations separately (fit from different parts of the CMD).
If MegaBEAST is fitting distances from the full CMD, then my comment can be ignored. Does that help?
from megabeast.
Yes, this helps. I think I will close this issue for now. If once we get the v1.0 of the megabeast running and this is an issue we do need to address, then we can reopen this issue or open another.
from megabeast.
Related Issues (20)
- code testing HOT 1
- Update to latest package template files HOT 1
- Infrastructure updates notice from Astropy Project HOT 1
- Incorrect pixel coordinates in naive map script HOT 3
- Move core computations to a callable function HOT 1
- Limit fitting to specific regions in HR space
- Full megabeast ensemble model
- Completeness specific to source density
- Full nD simulations
- Single population megabeast
- Off field for ensemble model
- MNT: Stop using ci-helpers in appveyor.yml HOT 1
- Mixture Model Ideas HOT 2
- Variable Model Uncertainties/Weights HOT 1
- Cuts to remove dusty AGB failure mode for making A_V maps
- Speedup when star parameters are fixed
- Move simulations to MegaBEAST
- Tests
- Assumed file name may result in an error when generating naive maps HOT 1
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