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...

תיאור מלא

מידע ביבליוגרפי
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
פורמט: Journal article
שפה:English
יצא לאור: American Astronomical Society 2019