Figure 5 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 5.

Comparison of temperatures derived using EW-based estimates from Newton et al. (2015) and spectral indices from Mann et al. (2013b) in J band (left), H band (middle), and K band (right). Points within the shaded region lie within 150 K of a one-to-one relation (solid line). All points are color-coded by [Fe/H], as indicated by the colorbar.

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