Christina Hedges

I saw there is a WIP to add `SecondaryEclipseLightCurve` to `exoplanet`, but that it doesn't include reflected/thermal phase curve light. I added a silly approximation to quickly add in a...

Should `search_tesscut` log a warning if a TPF is returned that contains collateral pixels?

2

When users try to download TESSCut data for targets such as `TIC 118555907`, they can be returned a TPF that will look and behave like regular data, but will actually...

Perhaps `SearchResult.download()` should accept an author "priority" order

5

Currently in lightkurve we have this awesome feature of being able to get light curves from different authors:  This is great! Sometimes I want to get a lot of...

Bin Function won't bin by a number of points

3

I'm finding it very hard to bin by a number of points in lightkurve right now. This used to be the default argument, but now the default argument is a...

lightkurve could take advantage of `np.ma.masked_arrays` and astropy's masked tables when quality masking

2

At the moment, `lightkurve` objects have a `quality` variable. This is a bit of an odd part of the object, because e.g. `tp.time` and `tpf.flux` will have one length, but...

`SparseDesignMatrix.split([...])` removes columns that are all zero automatically, but `DesignMatrix.split([...])` does not In `SparseDesignMatrixs.split` we have code around this line that finds all the components of the design matrix that...

Some of our dependencies should be optional (e.g. `scikit-learn`, `oktopus`)

3

I believe we currently have dependencies like `scikit-learn` and `oktopus` that are great packages and super useful, but only in certain contexts (`CBVCorrector` for example is the only module that...

In the `prf` module, users can plot the Kepler PRF model, and can use the `scale` keywords to "zoom in" on the PRF. However, when we plot it, it doesn't...

RegressionCorrector and DesignMatrix accept the new units on time and flux, but massively slow down.

1

In lightkurve 2.03b+ we have units on time, flux and flux error, and `time` is now an astropy Time object. These values can be passed into e.g. `lk.design_matrix.create_spline_matrix` or `lk.design_matrix.create_sparse_spline_matrix`,...

Would be helpful for planet vetting. Same as keppixseries. For K2 this should be detrendable for every pixel.