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The Kepler and K2 CBV time stamps on MAST are not barycenter corrected. Whereas the POC light curves on MAST *are* barycenter corrected. This causes a minor issue where the light curves and the CBVs a…
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Can you suggest a strategy how to efficiently find transits for light curves with long gap e.g. 1 year as in the case of EPICs observed in K2 Campaign 16 and again in C18? I may perhaps limit the peri…
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Beyond the objects that were targeted by K2, many objects moved through the K2 focal plane during observations that were not specifically targeted. This is particularly interesting in superstamps, whe…
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Hi @barentsen,
I am facing a similar problem with downloading data from K2 with the following:
`lk.search_targetpixelfile('EPIC228164766',mission='K2')`
> No data was found for target "EPIC2281…
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This issue is a final wrap up of the Kepler-Focus Lightkurve Tutorial project, which created 21 new Lightkurve tutorials. The tutorials were merged to the [STScI notebook repository](https://github.co…
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I wonder if we can have `kepstitch` take the name of a planet or KIC number, and have to grab all the quarters for that target from MAST and stitch it all together, so a user can obtain a full-mission…
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##### Description
The EPIC Variability Extraction and Removal for Exoplanet Science Targets (EVEREST) pipeline "de-trends K2 light curves with pixel level decorrelation and Gaussian processes". Th…
gully updated
6 years ago
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Asteroseismology can unlock stellar properties such as mass and radius independently from other methods. Until recently, asteroseismic analyses were only carried out in the frequency domain, by using …
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- [x] KRC find spectral models, send to JRAD
(The R~10,000 model grid at http://phoenix.astro.physik.uni-goettingen.de/?page_id=16 would be my recommended starting point)
## Pre NYC HW
- [ ] KRC fi…
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#### Problem description
If I run PLDCorrector on the same target pixel file to generate a light curve more than once, I get different value, different enough that fitting algorithms (e.g., scipy cur…