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_Issue [JP-3745](https://jira.stsci.edu/browse/JP-3745) was created on JIRA by [Aarynn Carter](https://jira.stsci.edu/secure/ViewProfile.jspa?name=aacarter):_
BACKGROUND: For NIRISS SOSS data, the …
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##### Description
K2 has observed over 40,000 galaxies anticipating ~50-100 Supernova outbursts. Instrumental artifacts arising from spacecraft motion have hindered the unambiguous census of trans…
gully updated
6 years ago
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##### Description
You only understand your data to the extent that you understand its generating process. The generative process of Kepler/K2 photometric time series data includes both instrumenta…
gully updated
6 years ago
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Running parameter estimation is the only sure-fire way to guarantee that DeepClean is, at the very least, not introducing noise into the strain or removing astrophysical signals. However, achieving st…
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This will probably involve integrations with `ml4gw`, but I'm realizing more and more that our default behavior of centering injections and treating the `trigger_offset` symmetrically probably doesn't…
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Here the limits from HESS
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I wouldn't dignify these with the term "candidates" but in the pound stars folder, I've put a zipped "gallery" of png images of the two most promising signals for each "pound star" (i.e. 72 bright, lo…
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I recently had another look at f3 and wondered about conceivable extensions and applications.
### Is it possible to calibrate the C5, C16, C18 FFIs in the same way as the Kepler prime mission?
As…
gully updated
4 years ago
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I'm delighted to see Goldilocks moving towards automated telluric corrections! 🎆 This is awesome! Here are a few thoughts:
### Minor comments
- `LDLS` -- what does the acronym stand for?
>t…
gully updated
3 years ago
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This needs to be fixed for the sake of imaging properly
I know MeerKAT uses something called Wishart noise statistics based on the autocorrelations. @tmolteno do we get correct autos out of the tel…