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These modules should be moved to analysis sub-package:
`temp_metallicity_calc` - Requires `hotfix/v0.6.2` rebase before fix. [5d2587f]
`ratios` - Require `hotfix/v0.6.2` for consistency. [5d2587f]
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This is intended to simplify individual_detection.py with a more generalized code. The code of interest is available [here](https://github.com/astrochun/Metallicity_Stack_Commons/blob/feature/composi…
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Hi,
This is a question to understand more of how Prospector v0.3.0 is doing cosmological dimming via 'zred' and/or 'lumindist' parameters in model dictionaries.
I am currently using Prospector…
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Hello!
First, I want to thank you for such a great package. Overall it is extremely well done and versatile.
However, I ran into an issue when I tried to use the Parsec isochrones. When attempti…
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At the moment SFR and Z calculations for the MC chains are done on the fly and significantly delay output. This should be done as a postprocessing step.
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![image (2)](https://user-images.githubusercontent.com/512213/78326222-93637f80-75c5-11ea-821f-374b01e55c7a.png)
Coen identified that the CO core mass can drop during stellar type transition (see p…
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Hi,
I am using Prospector (0.3.0) and python-FSPS (0.3.0) to test IGM absorption at redshifts greater than 3.5, using a CSpecBasis sps object, and an SSP (sfh=0) model with dust and subsolar metall…
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Changing naming convention so that tables/dictionaries created by MZEvolve and Zcalbase_gal have the same column names when allowed.
Also converting all table calls to dictionary calls.
Tables: …
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Hi, I'm trying to create a MCMC SED fitting pipeline using Python-fsps and emcee. My code initializes a single instance of the stellar population object as shown in the tutorial.
fsps.StellarPopula…
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We need A_V measurements for SDSS in order to:
- sample A_V directly for SFR = 0 population
- implement non-slab model that uses the A_V distribution