Figure 23 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 23.

Same as Figure 21 for hotter dwarfs with spectral types between K5 and K3. Although some of these stars were expected to be cool enough for the Newton et al. (2015) relations, they were assigned temperatures hotter than 4800 K and were therefore excluded from the cool dwarf analysis.

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