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M dwarfs tess #33
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M dwarfs tess #33
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Check out this pull request on See visual diffs & provide feedback on Jupyter Notebooks. Powered by ReviewNB |
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This is a great intro. Make sure to add some links to background information about M Dwarfs. Also it would be cool to link to a paper on the habitability of planets around M Dwarfs, my quick google search yielded this paper: https://doi.org/10.48550/arXiv.2203.10127
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You should briefly describe what's in the other notebook (~1-2 sentences), then put a [link here]. I'll make sure that when the notebooks go live, an appropriate link is added
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Having read through this section, I think you should motivate iterating through the "removing variability" steps. Why are we cleaning twice?
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This cleaned data looks.... ok. The first lightcurve in the list actually looks a little better to my eye; is there a reason you went with this one?
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@ttdu this lightcurve was one of the lightcurves with more easily parseable periodograms. I could mention this in the intro, if that's helpful!
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Line #2. sigma_2 = convolve(np.square(cleaned_twice - running_mean), g)
This 'g' factor does not appear in the notebook, so this cell failed when I ran it.
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It looks like some extra-long flares are getting marked twice. Should we perhaps raise our standards to 8 or 10 minutes? Or would this exclude too many flares?
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@arjunsavel , Please give another round of polish taking into account Tom and my comments. |
Short notebook for finding flares in TESS — related to the HST M dwarf notebook, loosely.