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An Update to the EVEREST K2 Pipeline: Short Cadence, Saturated Stars, and Kepler-like Photometry Down to Kp = 15

Rodrigo Luger, Ethan Kruse, Daniel Foreman-Mackey et al., 2018. The Astronomical Journal 156(3), 99.

The EVEREST pipeline (pixel-level decorrelation) for K2 light curves, version 2.

MYS0D79RXE46N3D · mystery · click to copyMHD 139139, the "Random Transiter"Articledoi: 10.3847/1538-3881/aad230Checked against the original0

What it's used for here

An independent K2 light curve of the star, useful to test whether the dips survive a different reduction.

Cited by on this site 2 records

Cite it

Luger, R., Kruse, E., Foreman-Mackey, D., Agol, E., & Saunders, N. (2018). An Update to the EVEREST K2 Pipeline: Short Cadence, Saturated Stars, and Kepler-like Photometry Down to Kp = 15. The Astronomical Journal 156(3), 99. https://doi.org/10.3847/1538-3881/aad230
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