The K2 Bright Star Survey. I. Methodology and data release
While the Kepler mission was designed to look at tens of thousands of faint stars (V gsim 12), brighter stars that saturated the detector are important because they can be and have been observed very accurately by other instruments. By analyzing the unsaturated scattered-light "halo" aroun...
Main Authors: | Pope, BJS, White, TR, Farr, WM, Yu, J, Greklek-McKeon, M, Huber, D, Aerts, C, Aigrain, S, Bedding, TR, Boyajian, T, Creevey, OL, Hogg, DW |
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Format: | Journal article |
Language: | English |
Published: |
American Astronomical Society
2019
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