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This entails:
1. A top-level makefile that "curl -O"s the data -- the star model input files and so on -- into a data directory. (That is, don't check in these large files, refer to them in a makefil…
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From @mpgalleg comment on the Population Analysis Framework:
> I tried to follow the tutorial and ran into an error when trying to calculate the observable population of BBH mergers using a populat…
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Simple area-scaling metrics should obtain for many MW science cases, that correlate with (or are identical to) existing metrics. These cases should appear in Summary Table 2 in section 3 of the MW cha…
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Looking at your tutorials 7-Acessing Chempy paper 1 abundance tracks.ipynb
https://github.com/jan-rybizki/Chempy/blob/master/tutorials/7-Acessing%20Chempy%20paper%201%20abundance%20tracks.ipynb
The …
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I am trying to do the first WASP14 tutorial but have not been able to generate the hdf5 data yet.
I setup config file like the docs as shown .
```
# YAML configuration script
name: example_was…
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I'm working through the example provided for the function modelFitEMCEE (posted below). I have tried a few variations (i.e., excluding keywords) and tried loading in a model first, too. I am getting…
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reported by: peter
The following problem was reported by Alexei Baskin:
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Hello,
I am trying to run Cloudy for different AGN models, changing the incident continuum (nuF_nu) and hy…
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@YuichiHarikane noticed that Beagle predicts a broad range of Lya / Ha ratios as a function of ionization parameter and metallicity.
The table below reports the Lya/Ha ratio, and Ha/Hb ratios, for …
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Hi,
How does the input of metallicity ( logzsol ) work.
When I give
> sps = fsps.StellarPopulation(zcontinuous=1,logzsol=-0.4)
> iso = sps.isochrones()
>
In the output, I get
> age log(Z…
kh-kr updated
3 years ago
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p(M_r) -- after Equation 5 -- states M_r_min_obs, and M_r_max_obs,
outside of which p(M_r)==0; this is important for the normalization.
But it doesn't say what these limiting values are.
In particular…
HWRix updated
9 years ago