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

Matías I. Jones; Rafael Brahm; Nestor Espinoza; Songhu Wang; Avi Shporer; Thomas Henning; Andrés Jordán; Paula Sarkis; Leonardo A. Paredes; James Hodari-Sadiki; Todd Henry; Bryndis Cruz; Louise D. Nielsen; François Bouchy; Francesco Pepe; Damien Ségransan; Oliver Turner; Stéphane Udry; Maxime Marmier; Christophe Lovis; Gaspar Bakos; David Osip; Vincent Suc; Carl Ziegler; Andrei Tokovinin; Nick M. Law; Andrew W. Mann; Howard Relles; Karen A. Collins; Daniel Bayliss; Elyar Sedaghati; David W. Latham; Sara Seager; Joshua N. Winn; Jon M. Jenkins; Jeffrey C. Smith; Misty Davies; Peter Tenenbaum; Jason DIttmann; Andrew Vanderburg; Jessie L. Christiansen; Kari Haworth; John Doty; Gabor Furész; Greg Laughlin; Elisabeth Matthews; Ian Crossfield; Steve Howell; David Ciardi; Erica Gonzales; Rachel Matson; Charles Beichman; Joshua Schlieder

doi:10.1051/0004-6361/201834640

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

Matías I. Jones, Rafael Brahm, Nestor Espinoza, Songhu Wang, Avi Shporer, Thomas Henning, Andrés Jordán, Paula Sarkis, Leonardo A. Paredes, James Hodari-Sadiki, Todd Henry, Bryndis Cruz, Louise D. Nielsen, François Bouchy, Francesco Pepe, Damien Ségransan, Oliver Turner, Stéphane Udry, Maxime Marmier, Christophe LovisGaspar Bakos, David Osip, Vincent Suc, Carl Ziegler, Andrei Tokovinin, Nick M. Law, Andrew W. Mann, Howard Relles, Karen A. Collins, Daniel Bayliss, Elyar Sedaghati, David W. Latham, Sara Seager, Joshua N. Winn, Jon M. Jenkins, Jeffrey C. Smith, Misty Davies, Peter Tenenbaum, Jason DIttmann, Andrew Vanderburg, Jessie L. Christiansen, Kari Haworth, John Doty, Gabor Furész, Greg Laughlin, Elisabeth Matthews, Ian Crossfield, Steve Howell, David Ciardi, Erica Gonzales, Rachel Matson, Charles Beichman, Joshua Schlieder

Research output: Contribution to journal › Article › peer-review

35 Scopus citations

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.

Original language	English
Article number	A16
Journal	Astronomy and Astrophysics
Volume	625
DOIs	https://doi.org/10.1051/0004-6361/201834640
State	Published - 1 May 2019
Externally published	Yes

Keywords

Instrumentation: spectrographs
Methods: observational
Planetary systems
Planets and satellites: detection
Techniques: radial velocities

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10.1051/0004-6361/201834640

Cite this

Jones, M. I., Brahm, R., Espinoza, N., Wang, S., Shporer, A., Henning, T., Jordán, A., Sarkis, P., Paredes, L. A., Hodari-Sadiki, J., Henry, T., Cruz, B., Nielsen, L. D., Bouchy, F., Pepe, F., Ségransan, D., Turner, O., Udry, S., Marmier, M., ... Schlieder, J. (2019). HD 2685 b: A hot Jupiter orbiting an early F-type star detected by TESS. Astronomy and Astrophysics, 625, Article A16. https://doi.org/10.1051/0004-6361/201834640

@article{8e9dea371109449d8ac7756cc7f4ba22,

title = "HD 2685 b: A hot Jupiter orbiting an early F-type star detected by TESS",

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.",

keywords = "Instrumentation: spectrographs, Methods: observational, Planetary systems, Planets and satellites: detection, Techniques: radial velocities",

author = "Jones, {Mat{\'i}as I.} and Rafael Brahm and Nestor Espinoza and Songhu Wang and Avi Shporer and Thomas Henning and Andr{\'e}s Jord{\'a}n and Paula Sarkis and Paredes, {Leonardo A.} and James Hodari-Sadiki and Todd Henry and Bryndis Cruz and Nielsen, {Louise D.} and Fran{\c c}ois Bouchy and Francesco Pepe and Damien S{\'e}gransan and Oliver Turner and St{\'e}phane Udry and Maxime Marmier and Christophe Lovis and Gaspar Bakos and David Osip and Vincent Suc and Carl Ziegler and Andrei Tokovinin and Law, {Nick M.} and Mann, {Andrew W.} and Howard Relles and Collins, {Karen A.} and Daniel Bayliss and Elyar Sedaghati and Latham, {David W.} and Sara Seager and Winn, {Joshua N.} and Jenkins, {Jon M.} and Smith, {Jeffrey C.} and Misty Davies and Peter Tenenbaum and Jason DIttmann and Andrew Vanderburg and Christiansen, {Jessie L.} and Kari Haworth and John Doty and Gabor Fur{\'e}sz and Greg Laughlin and Elisabeth Matthews and Ian Crossfield and Steve Howell and David Ciardi and Erica Gonzales and Rachel Matson and Charles Beichman and Joshua Schlieder",

note = "Publisher Copyright: {\textcopyright} ESO 2019.",

year = "2019",

month = may,

day = "1",

doi = "10.1051/0004-6361/201834640",

language = "English",

volume = "625",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Jones, MI, Brahm, R, Espinoza, N, Wang, S, Shporer, A, Henning, T, Jordán, A, Sarkis, P, Paredes, LA, Hodari-Sadiki, J, Henry, T, Cruz, B, Nielsen, LD, Bouchy, F, Pepe, F, Ségransan, D, Turner, O, Udry, S, Marmier, M, Lovis, C, Bakos, G, Osip, D, Suc, V, Ziegler, C, Tokovinin, A, Law, NM, Mann, AW, Relles, H, Collins, KA, Bayliss, D, Sedaghati, E, Latham, DW, Seager, S, Winn, JN, Jenkins, JM, Smith, JC, Davies, M, Tenenbaum, P, DIttmann, J, Vanderburg, A, Christiansen, JL, Haworth, K, Doty, J, Furész, G, Laughlin, G, Matthews, E, Crossfield, I, Howell, S, Ciardi, D, Gonzales, E, Matson, R, Beichman, C & Schlieder, J 2019, 'HD 2685 b: A hot Jupiter orbiting an early F-type star detected by TESS', Astronomy and Astrophysics, vol. 625, A16. https://doi.org/10.1051/0004-6361/201834640

TY - JOUR

T1 - HD 2685 b

T2 - A hot Jupiter orbiting an early F-type star detected by TESS

AU - Jones, Matías I.

AU - Brahm, Rafael

AU - Espinoza, Nestor

AU - Wang, Songhu

AU - Shporer, Avi

AU - Henning, Thomas

AU - Jordán, Andrés

AU - Sarkis, Paula

AU - Paredes, Leonardo A.

AU - Hodari-Sadiki, James

AU - Henry, Todd

AU - Cruz, Bryndis

AU - Nielsen, Louise D.

AU - Bouchy, François

AU - Pepe, Francesco

AU - Ségransan, Damien

AU - Turner, Oliver

AU - Udry, Stéphane

AU - Marmier, Maxime

AU - Lovis, Christophe

AU - Bakos, Gaspar

AU - Osip, David

AU - Suc, Vincent

AU - Ziegler, Carl

AU - Tokovinin, Andrei

AU - Law, Nick M.

AU - Mann, Andrew W.

AU - Relles, Howard

AU - Collins, Karen A.

AU - Bayliss, Daniel

AU - Sedaghati, Elyar

AU - Latham, David W.

AU - Seager, Sara

AU - Winn, Joshua N.

AU - Jenkins, Jon M.

AU - Smith, Jeffrey C.

AU - Davies, Misty

AU - Tenenbaum, Peter

AU - DIttmann, Jason

AU - Vanderburg, Andrew

AU - Christiansen, Jessie L.

AU - Haworth, Kari

AU - Doty, John

AU - Furész, Gabor

AU - Laughlin, Greg

AU - Matthews, Elisabeth

AU - Crossfield, Ian

AU - Howell, Steve

AU - Ciardi, David

AU - Gonzales, Erica

AU - Matson, Rachel

AU - Beichman, Charles

AU - Schlieder, Joshua

PY - 2019/5/1

Y1 - 2019/5/1

N2 - 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.

AB - 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.

KW - Instrumentation: spectrographs

KW - Methods: observational

KW - Planetary systems

KW - Planets and satellites: detection

KW - Techniques: radial velocities

UR - http://www.scopus.com/inward/record.url?scp=85103691285&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/201834640

DO - 10.1051/0004-6361/201834640

M3 - Article

AN - SCOPUS:85103691285

SN - 0004-6361

VL - 625

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A16

ER -

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

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Keywords

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