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I am using BADASS for another project where I have to extract [OIII] kinematics from Keck KCWI-Blue data (FWHM ~0.950 A from 4600-5700A).
While the VC04 optical FeII template has been working fine …
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Hi,
I am trying to fit a TESS light curve of an eclipsing binary. The parameter list is as follows
lc_initial = {
'system': {
# setting a reasonable expected starting value and ran…
kh-kr updated
2 years ago
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$ python3 plot_detailed_evolution.py
Time (Myr), Event, M1 (M_o), type1, M2 (M_o), type2, a (R_o), e
0.000000 Zero-age main-sequence, metallicity Z=0.0142 1.826 …
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My first run of this notebook was missing `gollum` as it's only listed in the `docs/requirements.txt` file, which is fine. I installed with `pip install gollum` (I didn't use the full `docs/requiremen…
wtgee updated
2 years ago
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I realized in past test runs I had forgotten to pass the model parameter for describing the fraction of blue horizontal branch stars (fBHB) in my stellar population so it had been fixed at the default…
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Hello! I'm really excited to use fastpp, but I'm really confused as to a few things with respect to the comparison between the results from fastpp and FAST-IDL. When I use the same parameter file with…
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**Describe the bug**
The mass transfer flag happens later than the mass transfer, leading to misleading detailed output.
**Label the issue**
`urgency_moderate` - This is a moderately urgent issu…
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It would be really nice to have a "global" filter that applies a filter onto all different particle types. For example, if we're looking at gas particles broken down into two classifications it would …
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I haven't come across anything in the documentation that directly addresses Population II and Population III stars, but I am interested in generating mock galaxies using one or both of these Populatio…
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Hi. I'm just beginning to play around with Picaso. I wanted to compute a reflected light spectrum of Earth. So, following the "Getting Started : Basic Inputs and Outputs" in the docs, I put together a…