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Hello, I'm a student from UT joining this project for summer 2022. To answer the above question, here are some tasks I'll need to accomplish:
- [x] Get the reduced IGRINS data @gully
- [x] Start …
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Can we reproduce the offsets seen in rapidly vs slowly rotating stars in the optical, based on their Kepler spot properties?
Requires Issue #2 to be built first
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Currently the code can model single stars with starspots @gully (with a single temp. and fill factor). We (@tofflemire, @gully and @edgillen) want to extend that to do full modelling of intrinsic (e.g…
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As with many exoplanet ideas, there is cross-fertilization with stellar astrophysics. The starry formalism could perhaps be used in mapping pulsations of stars in eclipsing binaries during eclipses:
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I had an idea while watching a [video on Gibbs sampling](http://videolectures.net/mlss09uk_murray_mcmc/) (the bit beginning at roughly 1h09m): Maybe we can adapt the Gibbs sampler to deal with correl…
gully updated
8 years ago
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Hi folks, I recently emailed some Starfish quick start notes to a colleague, and thought I'd post them here in case they are useful to anyone else. More tips/tricks for newcomers are welcomed below.
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gully updated
7 years ago
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The `welter` outline resides in `document/README.md`. Consider updating this outline to the present document.
gully updated
6 years ago
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The current EDDis program has about 3/4 of its size in a 27 MB icon-assembly, consisting mostly of png resources. I see that many of the files have already been quantized to 256 indexed colors, the st…
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### 1. Attributing the Helium signal to planet rather than activity
Suvrath asked about attributing the signal to planetary mass loss and not stellar variability. At face value, many of the obser…