HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS

Songhu Wang; Matias Jones; Avi Shporer; Benjamin J. Fulton; Leonardo A. Paredes; Trifon Trifonov; Diana Kossakowski; Jason Eastman; Seth Redfield; Maximilian N. Günther; Laura Kreidberg; Chelsea X. Huang; Sarah Millholland; Darryl Seligman; Debra Fischer; Rafael Brahm; Xian Yu Wang; Bryndis Cruz; Todd Henry; Hodari Sadiki James; Brett Addison; En Si Liang; Allen B. Davis; René Tronsgaard; Keduse Worku; John M. Brewer; Martin Kürster; Hui Zhang; Charles A. Beichman; Allyson Bieryla; Timothy M. Brown; Jessie L. Christiansen; David R. Ciardi; Karen A. Collins; Gilbert A. Esquerdo; Andrew W. Howard; Howard Isaacson; David W. Latham; Tsevi Mazeh; Erik A. Petigura; Samuel N. Quinn; Sahar Shahaf; Robert J. Siverd; Florian Rodler; Sabine Reffert; Olga Zakhozhay; George R. Ricker; Roland Vanderspek; Sara Seager; Joshua N. Winn; Jon M. Jenkins; Patricia T. Boyd; Gábor Frész; Christopher Henze; Alen M. Levine; Robert Morris; Martin Paegert; Keivan G. Stassun; Eric B. Ting; Michael Vezie; Gregory Laughlin

doi:10.3847/1538-3881/aaf1b7

HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS

Songhu Wang
, Matias Jones
, Avi Shporer
, Benjamin J. Fulton
, Leonardo A. Paredes
, Trifon Trifonov
, Diana Kossakowski
, Jason Eastman
, Seth Redfield
, Maximilian N. Günther
, Laura Kreidberg
, Chelsea X. Huang
, Sarah Millholland
, Darryl Seligman
, Debra Fischer
, Rafael Brahm
, Xian Yu Wang
, Bryndis Cruz
, Todd Henry
, Hodari Sadiki James

Brett Addison, En Si Liang, Allen B. Davis, René Tronsgaard, Keduse Worku, John M. Brewer, Martin Kürster, Hui Zhang, Charles A. Beichman, Allyson Bieryla, Timothy M. Brown, Jessie L. Christiansen, David R. Ciardi, Karen A. Collins, Gilbert A. Esquerdo, Andrew W. Howard, Howard Isaacson, David W. Latham, Tsevi Mazeh, Erik A. Petigura, Samuel N. Quinn, Sahar Shahaf, Robert J. Siverd, Florian Rodler, Sabine Reffert, Olga Zakhozhay, George R. Ricker, Roland Vanderspek, Sara Seager, Joshua N. Winn, Jon M. Jenkins, Patricia T. Boyd, Gábor Frész, Christopher Henze, Alen M. Levine, Robert Morris, Martin Paegert, Keivan G. Stassun, Eric B. Ting, Michael Vezie, Gregory Laughlin

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

71 Citas (Scopus)

Resumen

We report the first confirmation of a hot Jupiter discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HD 202772A b. The transit signal was detected in the data from TESS Sector 1, and was confirmed to be of planetary origin through radial velocity (RV) measurements. HD 202772A b is orbiting a mildly evolved star with a period of 3.3 days. With an apparent magnitude of V = 8.3, the star is among the brightest and most massive known to host a hot Jupiter. Based on the 27 days of TESS photometry and RV data from the CHIRON, HARPS, and Tillinghast Reflector Echelle Spectrograph, the planet has a mass of and radius of , making it an inflated gas giant. HD 202772A b is a rare example of a transiting hot Jupiter around a quickly evolving star. It is also one of the most strongly irradiated hot Jupiters currently known.

Idioma original	Inglés
Número de artículo	51
Publicación	Astronomical Journal
Volumen	157
N.º	2
DOI	https://doi.org/10.3847/1538-3881/aaf1b7
Estado	Publicada - feb 2019
Publicado de forma externa	Sí

Acceder al documento

10.3847/1538-3881/aaf1b7

Citar esto

Wang, S., Jones, M., Shporer, A., Fulton, B. J., Paredes, L. A., Trifonov, T., Kossakowski, D., Eastman, J., Redfield, S., Günther, M. N., Kreidberg, L., Huang, C. X., Millholland, S., Seligman, D., Fischer, D., Brahm, R., Wang, X. Y., Cruz, B., Henry, T., ... Laughlin, G. (2019). HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS. Astronomical Journal, 157(2), Artículo 51. https://doi.org/10.3847/1538-3881/aaf1b7

@article{b956b9cc38d5423d9e7fcb1156158632,

title = "HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS",

abstract = "We report the first confirmation of a hot Jupiter discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HD 202772A b. The transit signal was detected in the data from TESS Sector 1, and was confirmed to be of planetary origin through radial velocity (RV) measurements. HD 202772A b is orbiting a mildly evolved star with a period of 3.3 days. With an apparent magnitude of V = 8.3, the star is among the brightest and most massive known to host a hot Jupiter. Based on the 27 days of TESS photometry and RV data from the CHIRON, HARPS, and Tillinghast Reflector Echelle Spectrograph, the planet has a mass of and radius of , making it an inflated gas giant. HD 202772A b is a rare example of a transiting hot Jupiter around a quickly evolving star. It is also one of the most strongly irradiated hot Jupiters currently known.",

keywords = "planetary systems, planets and satellites: detection, stars: individual (TIC 290131778-TOI 123-HD 202772, techniques: radial velocities",

author = "Songhu Wang and Matias Jones and Avi Shporer and Fulton, \{Benjamin J.\} and Paredes, \{Leonardo A.\} and Trifon Trifonov and Diana Kossakowski and Jason Eastman and Seth Redfield and G{\"u}nther, \{Maximilian N.\} and Laura Kreidberg and Huang, \{Chelsea X.\} and Sarah Millholland and Darryl Seligman and Debra Fischer and Rafael Brahm and Wang, \{Xian Yu\} and Bryndis Cruz and Todd Henry and James, \{Hodari Sadiki\} and Brett Addison and Liang, \{En Si\} and Davis, \{Allen B.\} and Ren{\'e} Tronsgaard and Keduse Worku and Brewer, \{John M.\} and Martin K{\"u}rster and Hui Zhang and Beichman, \{Charles A.\} and Allyson Bieryla and Brown, \{Timothy M.\} and Christiansen, \{Jessie L.\} and Ciardi, \{David R.\} and Collins, \{Karen A.\} and Esquerdo, \{Gilbert A.\} and Howard, \{Andrew W.\} and Howard Isaacson and Latham, \{David W.\} and Tsevi Mazeh and Petigura, \{Erik A.\} and Quinn, \{Samuel N.\} and Sahar Shahaf and Siverd, \{Robert J.\} and Florian Rodler and Sabine Reffert and Olga Zakhozhay and Ricker, \{George R.\} and Roland Vanderspek and Sara Seager and Winn, \{Joshua N.\} and Jenkins, \{Jon M.\} and Boyd, \{Patricia T.\} and G{\'a}bor Fr{\'e}sz and Christopher Henze and Levine, \{Alen M.\} and Robert Morris and Martin Paegert and Stassun, \{Keivan G.\} and Ting, \{Eric B.\} and Michael Vezie and Gregory Laughlin",

year = "2019",

month = feb,

doi = "10.3847/1538-3881/aaf1b7",

language = "English",

volume = "157",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

number = "2",

}

Wang, S, Jones, M, Shporer, A, Fulton, BJ, Paredes, LA, Trifonov, T, Kossakowski, D, Eastman, J, Redfield, S, Günther, MN, Kreidberg, L, Huang, CX, Millholland, S, Seligman, D, Fischer, D, Brahm, R, Wang, XY, Cruz, B, Henry, T, James, HS, Addison, B, Liang, ES, Davis, AB, Tronsgaard, R, Worku, K, Brewer, JM, Kürster, M, Zhang, H, Beichman, CA, Bieryla, A, Brown, TM, Christiansen, JL, Ciardi, DR, Collins, KA, Esquerdo, GA, Howard, AW, Isaacson, H, Latham, DW, Mazeh, T, Petigura, EA, Quinn, SN, Shahaf, S, Siverd, RJ, Rodler, F, Reffert, S, Zakhozhay, O, Ricker, GR, Vanderspek, R, Seager, S, Winn, JN, Jenkins, JM, Boyd, PT, Frész, G, Henze, C, Levine, AM, Morris, R, Paegert, M, Stassun, KG, Ting, EB, Vezie, M & Laughlin, G 2019, 'HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS', Astronomical Journal, vol. 157, n.º 2, 51. https://doi.org/10.3847/1538-3881/aaf1b7

TY - JOUR

T1 - HD 202772A b

T2 - A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS

AU - Wang, Songhu

AU - Jones, Matias

AU - Shporer, Avi

AU - Fulton, Benjamin J.

AU - Paredes, Leonardo A.

AU - Trifonov, Trifon

AU - Kossakowski, Diana

AU - Eastman, Jason

AU - Redfield, Seth

AU - Günther, Maximilian N.

AU - Kreidberg, Laura

AU - Huang, Chelsea X.

AU - Millholland, Sarah

AU - Seligman, Darryl

AU - Fischer, Debra

AU - Brahm, Rafael

AU - Wang, Xian Yu

AU - Cruz, Bryndis

AU - Henry, Todd

AU - James, Hodari Sadiki

AU - Addison, Brett

AU - Liang, En Si

AU - Davis, Allen B.

AU - Tronsgaard, René

AU - Worku, Keduse

AU - Brewer, John M.

AU - Kürster, Martin

AU - Zhang, Hui

AU - Beichman, Charles A.

AU - Bieryla, Allyson

AU - Brown, Timothy M.

AU - Christiansen, Jessie L.

AU - Ciardi, David R.

AU - Collins, Karen A.

AU - Esquerdo, Gilbert A.

AU - Howard, Andrew W.

AU - Isaacson, Howard

AU - Latham, David W.

AU - Mazeh, Tsevi

AU - Petigura, Erik A.

AU - Quinn, Samuel N.

AU - Shahaf, Sahar

AU - Siverd, Robert J.

AU - Rodler, Florian

AU - Reffert, Sabine

AU - Zakhozhay, Olga

AU - Ricker, George R.

AU - Vanderspek, Roland

AU - Seager, Sara

AU - Winn, Joshua N.

AU - Jenkins, Jon M.

AU - Boyd, Patricia T.

AU - Frész, Gábor

AU - Henze, Christopher

AU - Levine, Alen M.

AU - Morris, Robert

AU - Paegert, Martin

AU - Stassun, Keivan G.

AU - Ting, Eric B.

AU - Vezie, Michael

AU - Laughlin, Gregory

PY - 2019/2

Y1 - 2019/2

N2 - We report the first confirmation of a hot Jupiter discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HD 202772A b. The transit signal was detected in the data from TESS Sector 1, and was confirmed to be of planetary origin through radial velocity (RV) measurements. HD 202772A b is orbiting a mildly evolved star with a period of 3.3 days. With an apparent magnitude of V = 8.3, the star is among the brightest and most massive known to host a hot Jupiter. Based on the 27 days of TESS photometry and RV data from the CHIRON, HARPS, and Tillinghast Reflector Echelle Spectrograph, the planet has a mass of and radius of , making it an inflated gas giant. HD 202772A b is a rare example of a transiting hot Jupiter around a quickly evolving star. It is also one of the most strongly irradiated hot Jupiters currently known.

AB - We report the first confirmation of a hot Jupiter discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HD 202772A b. The transit signal was detected in the data from TESS Sector 1, and was confirmed to be of planetary origin through radial velocity (RV) measurements. HD 202772A b is orbiting a mildly evolved star with a period of 3.3 days. With an apparent magnitude of V = 8.3, the star is among the brightest and most massive known to host a hot Jupiter. Based on the 27 days of TESS photometry and RV data from the CHIRON, HARPS, and Tillinghast Reflector Echelle Spectrograph, the planet has a mass of and radius of , making it an inflated gas giant. HD 202772A b is a rare example of a transiting hot Jupiter around a quickly evolving star. It is also one of the most strongly irradiated hot Jupiters currently known.

KW - planetary systems

KW - planets and satellites: detection

KW - stars: individual (TIC 290131778-TOI 123-HD 202772

KW - techniques: radial velocities

UR - https://www.scopus.com/pages/publications/85060998297

U2 - 10.3847/1538-3881/aaf1b7

DO - 10.3847/1538-3881/aaf1b7

M3 - Article

AN - SCOPUS:85060998297

SN - 0004-6256

VL - 157

JO - Astronomical Journal

JF - Astronomical Journal

IS - 2

M1 - 51

ER -

HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS

Resumen

Acceder al documento

Huella

Citar esto