WASP-121b optical phase curve

Bourrier V.; Kitzmann D.; Kuntzer T.; Nascimbeni V.; Lendl M.; Lavie B.; Hoeijmakers H.J.; Pino L.; Ehrenreich D.; Heng K.; Allart R.; Cegla H.M; Dumusque X.; Melo C.; Astudillo-Defru, Nicola; Caldwell D.A.; Cretignier M.; Giles H.; Henze C.E.; Jenkins J.; Lovis C.; Murgas F.; Pepe F.; Ricker G.R.; Rose M.E.; Seager S.; Segransan D.; Suarez-Mascareno A.; Udry S.; Vanderspek R.; Wyttenbach A.

doi:10.26093/cds/vizier.36370036

Título

WASP-121b optical phase curve

Fecha

2020

Autores

Bourrier V.

Kitzmann D.

Kuntzer T.

Nascimbeni V.

Lendl M.

Lavie B.

Hoeijmakers H.J.

Pino L.

Ehrenreich D.

Heng K.

DOI

10.26093/cds/vizier.36370036

Resumen

Binned TESS light curve of WASP-121b, phase-folded at the orbital period of the planet. The flux is normalized to unity during the secondary eclipse, when the stellar light alone is measured.

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WASP-121b optical phase curve.zip

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