KeplerGO/lightkurve: Lightkurve v1.3.0

Published October 21, 2019 | Version v1.3.0

Software Open

1. NASA
2. K2 GO Office
3. HKUST@ConvexGroup
4. University of Hawaii
5. Kepler/K2 GO Office at NASA Ames Research Center
6. DIRAC Institute, University of Washington
7. Self-employed
8. Center for Astrophysics | Harvard & Smithsonian and the American Astronomical Society
9. UoB
10. University of Sydney
11. @Zocdoc

Lightkurve v1.3.0 includes the following changes:

Added a method="quadratic" option to tpf.estimate_centroids() which enables centroids to be estimated by fitting a bivariate polynomial to the 3x3 pixel core of the PSF. The method can also be called as a standalone function via lightkurve.utils.centroid_quadratic(). [#544, #610]
Fixed a bug in Seismology.plot_echelle() which caused the Echelle diagram of a power spectrum to be rendered incorrectly. [#602]
Fixed a bug which caused lightkurve.utils to be incorrectly resolved to lightkurve.seismology.utils. [#606]
Changed bkjd_to_astropy_time() and btjd_to_astropy_time() to accept a single float and lists of floats in addition to numpy arrays. [#608]
Improved support for creating a LombScarglePeriodogram with an unevenly sampled grid in frequency space. [#614]

Files

Name	Size	Download all
KeplerGO/lightkurve-v1.3.0.zip md5:8cb0f1ee0daabb2125e26f27e6d64c0c	32.3 MB	Preview Download

Citations

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