Figure 1 from Characterizing K2 Candidate Planetary Systems Orbiting Low-mass Stars. I. Classifying Low-mass Host Stars Observed during Campaigns 1

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Characterizing K2 Candidate Planetary Systems Orbiting Low-mass Stars. I. Classifying Low-mass Host Stars Observed during Campaigns 1–7

Authors: Courtney D. Dressing, Elisabeth R. Newton, Joshua E. Schlieder, David Charbonneau, Heather A. Knutson, and Andrew Vanderburg

2017 The Astrophysical Journal 836 167.

Provider: AAS Journals

Caption: Figure 1.

Magnitude distribution of our full target sample in the Kepler bandpass (Kp; blue) and Ks (red). Our targets have median brightnesses of Ks = 10.8 and Kp = 13.5. The Kepler bandpass extends from roughly 420 nm to 900 nm with maximum response at 575 nm (Van Cleve & Caldwell 2016); the Ks bandpass is centered at 2.159 μm (Cohen et al. 2003).

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