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HD 2685 b: a hot Jupiter orbiting an early F-type star detected by TESS

MPS-Authors

Jones,  Matías I.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Brahm,  Rafael
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Espinoza,  Nestor
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Wang,  Songhu
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Shporer,  Avi
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Henning,  Thomas
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Jordán,  Andrés
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Sarkis,  Paula
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Paredes,  Leonardo A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Hodari-Sadiki,  James
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Henry,  Todd
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Cruz,  Bryndis
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Nielsen,  Louise D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Bouchy,  François
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Pepe,  Francesco
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ségransan,  Damien
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Turner,  Oliver
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Udry,  Stéphane
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Marmier,  Maxime
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Lovis,  Christophe
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Bakos,  Gaspar
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Osip,  David
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Suc,  Vincent
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ziegler,  Carl
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tokovinin,  Andrei
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Law,  Nick M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Mann,  Andrew W.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Relles,  Howard
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Collins,  Karen A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Bayliss,  Daniel
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Sedaghati,  Elyar
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Latham,  David W.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Seager,  Sara
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Winn,  Joshua N.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Jenkins,  Jon M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Smith,  Jeffrey C.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Davies,  Misty
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tenenbaum,  Peter
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Dittmann,  Jason
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Vanderburg,  Andrew
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Christiansen,  Jessie L.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Haworth,  Kari
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Doty,  John
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Furész,  Gabor
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Laughlin,  Greg
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Matthews,  Elisabeth
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Crossfield,  Ian
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Howell,  Steve
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ciardi,  David
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Gonzales,  Erica
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Matson,  Rachel
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Beichman,  Charles
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Schlieder,  Joshua
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

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Citation

Jones, M. I., Brahm, R., Espinoza, N., Wang, S., Shporer, A., Henning, T., et al. (2019). HD 2685 b: a hot Jupiter orbiting an early F-type star detected by TESS. Astronomy and Astrophysics, 625.


Cite as: https://hdl.handle.net/21.11116/0000-0005-D357-B
Abstract
We report on the confirmation of a transiting giant planet around the relatively hot (Teff = 6801 ± 76 K) star HD 2685, whose transit signal was detected in Sector 1 data of NASA's TESS mission. We confirmed the planetary nature of the transit signal using Doppler velocimetric measurements with CHIRON, CORALIE, and FEROS, as well as using photometric data obtained with the Chilean-Hungarian Automated Telescope and the Las Cumbres Observatory. From the joint analysis of photometry and radial velocities, we derived the following parameters for HD 2685 b: P = 4.12688-0.00004+0.00005 days, e = 0.091-0.047+0.039, MP = 1.17 ± 0.12 MJ, and RP =1.44 ± 0.05 RJ. This system is a typical example of an inflated transiting hot Jupiter in a low- eccentricity orbit. Based on the apparent visual magnitude (V = 9.6 mag) of the host star, this is one of the brightest known stars hosting a transiting hot Jupiter, and it is a good example of the upcoming systems that will be detected by TESS during the two-year primary mission. This is also an excellent target for future ground- and space-based atmospheric characterization as well as a good candidate for measuring the projected spin-orbit misalignment angle through the Rossiter- McLaughlin effect. Tables of the photometry are only available at the CDS via anonymous ftp to <A href="http://cdsarc.u-strasbg.fr">http://cdsarc.u-strasbg.fr</A> (ftp://130.79.128.5) or via <A href="http://cdsarc.u-strasbg.fr/viz- bin/qcat?J/A+A/625/A16">http://cdsarc.u-strasbg.fr/viz- bin/qcat?J/A+A/625/A16</A>