Figure 1 from WASP-4b Arrived Early for the TESS Mission

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WASP-4b Arrived Early for the TESS Mission

Authors: L.G. Bouma, J.N. Winn, C. Baxter, W. Bhatti, F. Dai, T. Daylan, J.-M. Désert, M.L. Hill, S.R. Kane, K.G. Stassun, J. Villasenor, G.R. Ricker, R. Vanderspek, D.W. Latham, S. Seager, J.M. Jenkins, Z. Berta-Thompson, K. Colón, M. Fausnaugh, Ana Glidden, N. Guerrero, J.E. Rodriguez, J.D. Twicken, and B. Wohler

2019 The Astronomical Journal 157 217.

Provider: AAS Journals

Caption: Figure 1.

TESS observations of WASP-4b. On the left, black points are TESS flux measurements, with a vertical offset applied. Blue curves are best-fit models. The numbers printed next to each light curve are the approximate transit times expressed in BJD minus 2,457,000. The right side shows the residuals.

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