Figure 3 from Determining Empirical Stellar Masses and Radii from Transits and Gaia Parallaxes as Illustrated by Spitzer Observations of KELT-11b

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Determining Empirical Stellar Masses and Radii from Transits and Gaia Parallaxes as Illustrated by Spitzer Observations of KELT-11b

Authors: Thomas G. Beatty, Daniel J. Stevens, Karen A. Collins, Knicole D. Colón, David J. James, Laura Kreidberg, Joshua Pepper, Joseph E. Rodriguez, Robert J. Siverd, Keivan G. Stassun, and John F. Kielkopf

2017 The Astronomical Journal 154 25.

Provider: AAS Journals

Caption: Figure 3.

In addition to the Spitzer photometry, we also observed three new partial transits of KELT-11b using the ULMT telescope (Section 2.2). Here we have plotted the detrended new ULMT light curves, along with the best-fit transit model.

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