KeplerGO/lightkurve: Lightkurve v1.3.0
- Geert Barentsen1
- Christina Hedges2
- Zé Vinícius3
- Nicholas Saunders4
- gully5
- Oliver Hall
- Keaton Bell6
- Sheila Sagear
- Jose A Lerma III7
- Tom Barclay
- KenMighell
- Johnny Zhang
- Emma Turtelboom
- Ann Marie Cody
- Zach Berta-Thompson
- Sam Lee
- Peter Williams8
- Pal Szabo
- Guy Davies9
- Daniel10
- Brennan Vincello
- Anand Sundaram11
- 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
Description
Lightkurve v1.3.0 includes the following changes:
Added a
method="quadratic"option totpf.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 vialightkurve.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.utilsto be incorrectly resolved tolightkurve.seismology.utils. [#606]Changed
bkjd_to_astropy_time()andbtjd_to_astropy_time()to accept a single float and lists of floats in addition to numpy arrays. [#608]Improved support for creating a
LombScarglePeriodogramwith an unevenly sampled grid in frequency space. [#614]
Files
KeplerGO/lightkurve-v1.3.0.zip
Additional details
Related works
- Is supplement to
- https://github.com/KeplerGO/lightkurve/tree/v1.3.0 (URL)