-
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.
-
Coen identified that the CO core mass can drop during stellar type transition (see p…
-
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: …
-
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…
-
The nice utility `make_onezone_ray()` is for creating a ray with a single absorber element on it. This works fine in the `master` branch with the tip of yt's dev branch. However, there is a problem …
-
There may be an issue with LBV implementation: there does no appear to be a flattening of the remnant masses due to LBV winds at high ZAMS masses that is described, e.g., in the appendix to Neijssel+,…
-
Update column names in tables to common names provided in Metallicity_Stack_Commons to be consistent with MZEvolve and Zcalbase_gal.
Tables to be changed:
- binning.tbl --> implement:
- …
-
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
-
The module would be called `error_prop`
It will include:
1. [X] Construction of probability distribution functions (PDFs) based on inputs and 1-sigma uncertainties
2. [X] Calculation of 68-percen…
-
**Description**
I was reading about the missing "data parallelization" in SKIRT v9 on the [SKIRT update page](https://skirt.ugent.be/version9/_new_in_s_k_i_r_t9.html), and wondering what consequences…