Geert Barentsen
Geert Barentsen
This PR is a work in progress. cf. #918
This is a follow-up of #912. Several excellent sets of TESS community light curves are now available at MAST as High Level Science Products. We already support searching and opening...
When plotting SPOC and QLP light curves together using the following example: ```python import lightkurve as lk lk.search_lightcurve('TIC 1717079071', sector=26, radius=0.0001).download_all().plot() ``` The Y label says "Normalized Flux" based on...
This PR adds a `method='mean'` option to `LightCurve.normalize()` in response to #669.
Based on discussions with @danhey and @ojhall94 at the TASOC workshop this week, the idea has emerged to add `amplitude` and `psd` properties to `LombScarglePeriodogram` to enable anyone to use...
Example: ```python In [1]: import lightkurve as lk In [2]: tpf = lk.search_targetpixelfile("EPIC 211771334", campaign=18).download() In [3]: tpf.to_lightcurve(aperture_mask="threshold").to_corrector("sff").correct() /home/gb/bin/anaconda/lib/python3.7/site-packages/scipy/interpolate/interpolate.py:610: RuntimeWarning: divide by zero encountered in true_divide slope = (y_hi -...
As a convenient "container" for the various priors and likelihoods that we may want to use when carrying out PSF photometry, we should think about adding a `KeplerSceneModel` class. In...
Now that PyKE v3.1.0 is released, let's work towards a v.3.2.0 release in which the new API (i.e. the `LightCurve`, `KeplerTargetPixelFile`, `SFFCorrector`, .... classes) is removed in favor of a...
PyKE could offer to inject a planet signal using a very simple transit model. For more advanced transit models, we'd want to show in the documentation how the user can...
Right now, in `SFFCorrector`, we fit the motion polynomials as follows: ``` # Next, we fit the motion polynomial after removing outliers self.outlier_cent = sigma_clip(data=self.rot_col, sigma=sigma_2).mask coeffs = np.polyfit(self.rot_row[~self.outlier_cent], self.rot_col[~self.outlier_cent],...