Christina Hedges
Christina Hedges
Right now there are some problems with search which are only becoming apparent as we have more and more data from TESS; * Right now if you search for a...
#### Problem description When we take a subset of columns on a `LightCurve` object we should be able to bin a little faster (because there's less data to bin). At...
This PR fixes bugs in the `LightCurve`, `KeplerLightCurve`, and `TESSLightCurve` `to_fits` methods and the tests. This ensures users can pass extra keyword arguments. @Nschanche points out that it's odd that,...
Astropy tables have [`groups`](https://docs.astropy.org/en/stable/table/operations.html#id2) which can help split tables into different groups. We might benefit from giving users a way to separate into different orbits. Then users can split the...
#### Problem description Lightkurve's plot methods usually show plots inline in jupyter notebooks. Since v2.3 was released, I've noticed that sometimes plots do not render, and I have to use...
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, where...
As discussed in #17 and raised by @kstassun, "Flicker" noise is an excellent way to characterize stellar properties using photometric time series. Flicker noise occurs due to the granulation on...
Star clusters provide the opportunity to study stars that can be assumed to have the same age, composition, and formation history. We can use them as laboratories for understanding stellar...
The shape of an exoplanet transit provides critical information on the size and shape of the transiting object. Candidate objects that may exhibit different transit shapes, such as disintegrating planets,...
Investigating the frequency of planets around binary stars was one of Kepler’s prime mission goals, as binary stars and multi-star systems are common. Although some planets have been found to...