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

Research output: Contribution to journalJournal article – Annual report year: 2019Researchpeer-review

Standard

HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS. / Wang, Songhu; Jones, Matias; Shporer, Avi; Fulton, Benjamin J.; Paredes, Leonardo A.; Trifonov, Trifon; Kossakowski, Diana; Eastman, Jason; Redfield, Seth; Günther, Maximilian N.; Kreidberg, Laura; Huang, Chelsea X.; Millholland, Sarah; Seligman, Darryl; Fischer, Debra; Brahm, Rafael; Wang, Xian-Yu; Cruz, Bryndis; Henry, Todd; James, Hodari-Sadiki; Addison, Brett; Liang, En-Si; Davis, Allen B.; Tronsgaard, René; Worku, Keduse; Brewer, John M.; Kürster, Martin; Zhang, Hui; Beichman, Charles A.; Bieryla, Allyson; Brown, Timothy M.; Christiansen, Jessie L.; Ciardi, David R.; Collins, Karen A.; Esquerdo, Gilbert A.; Howard, Andrew W.; Isaacson, Howard; Latham, David W.; Mazeh, Tsevi; Petigura, Erik A.; Quinn, Samuel N.; Shahaf, Sahar; Siverd, Robert J.; Rodler, Florian; Reffert, Sabine; Zakhozhay, Olga; Ricker, George R.; Vanderspek, Roland; Seager, Sara; Winn, Joshua N.; Jenkins, Jon M.; T. Boyd, Patricia ; Fűrész, Gábor ; Henze, Christopher ; M. Levine, Alen ; Morris, Robert; Paegert, Martin ; G. Stassun, Keivan; B. Ting, Eric ; Vezie, Michael ; Laughlin, Gregory .

In: Astrophysical Journal, Vol. 157, No. 2, 51, 2019.

Research output: Contribution to journalJournal article – Annual report year: 2019Researchpeer-review

Harvard

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, X-Y, Cruz, B, Henry, T, James, H-S, Addison, B, Liang, E-S, 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, T. Boyd, P, Fűrész, G, Henze, C, M. Levine, A, Morris, R, Paegert, M, G. Stassun, K, B. Ting, E, 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', Astrophysical Journal, vol. 157, no. 2, 51. https://doi.org/10.3847/1538-3881/aaf1b7

APA

Wang, S., Jones, M., Shporer, A., Fulton, B. J., Paredes, L. A., Trifonov, T., ... Laughlin, G. (2019). HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS. Astrophysical Journal, 157(2), [51]. https://doi.org/10.3847/1538-3881/aaf1b7

CBE

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 X-Y, Cruz B, Henry T, James H-S, Addison B, Liang E-S, 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, T. Boyd P, Fűrész G, Henze C, M. Levine A, Morris R, Paegert M, G. Stassun K, B. Ting E, 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. Astrophysical Journal. 157(2). https://doi.org/10.3847/1538-3881/aaf1b7

MLA

Vancouver

Author

Wang, Songhu ; Jones, Matias ; Shporer, Avi ; Fulton, Benjamin J. ; Paredes, Leonardo A. ; Trifonov, Trifon ; Kossakowski, Diana ; Eastman, Jason ; Redfield, Seth ; Günther, Maximilian N. ; Kreidberg, Laura ; Huang, Chelsea X. ; Millholland, Sarah ; Seligman, Darryl ; Fischer, Debra ; Brahm, Rafael ; Wang, Xian-Yu ; Cruz, Bryndis ; Henry, Todd ; James, Hodari-Sadiki ; Addison, Brett ; Liang, En-Si ; Davis, Allen B. ; Tronsgaard, René ; Worku, Keduse ; Brewer, John M. ; Kürster, Martin ; Zhang, Hui ; Beichman, Charles A. ; Bieryla, Allyson ; Brown, Timothy M. ; Christiansen, Jessie L. ; Ciardi, David R. ; Collins, Karen A. ; Esquerdo, Gilbert A. ; Howard, Andrew W. ; Isaacson, Howard ; Latham, David W. ; Mazeh, Tsevi ; Petigura, Erik A. ; Quinn, Samuel N. ; Shahaf, Sahar ; Siverd, Robert J. ; Rodler, Florian ; Reffert, Sabine ; Zakhozhay, Olga ; Ricker, George R. ; Vanderspek, Roland ; Seager, Sara ; Winn, Joshua N. ; Jenkins, Jon M. ; T. Boyd, Patricia ; Fűrész, Gábor ; Henze, Christopher ; M. Levine, Alen ; Morris, Robert ; Paegert, Martin ; G. Stassun, Keivan ; B. Ting, Eric ; Vezie, Michael ; Laughlin, Gregory . / HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS. In: Astrophysical Journal. 2019 ; Vol. 157, No. 2.

Bibtex

@article{f8552e9e1b0147669713521b6abd6217,
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 1.017+0.070/- 0.068 MJ and radius of 1.545 +0.052/-0.060 RJ, 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 Xian-Yu Wang and Bryndis Cruz and Todd Henry and Hodari-Sadiki James and Brett Addison and En-Si Liang 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 {T. Boyd}, Patricia and G{\'a}bor Fűr{\'e}sz and Christopher Henze and {M. Levine}, Alen and Robert Morris and Martin Paegert and {G. Stassun}, Keivan and {B. Ting}, Eric and Michael Vezie and Gregory Laughlin",
year = "2019",
doi = "10.3847/1538-3881/aaf1b7",
language = "English",
volume = "157",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "IOP Publishing",
number = "2",

}

RIS

TY - JOUR

T1 - HD 202772A b: 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 - T. Boyd, Patricia

AU - Fűrész, Gábor

AU - Henze, Christopher

AU - M. Levine, Alen

AU - Morris, Robert

AU - Paegert, Martin

AU - G. Stassun, Keivan

AU - B. Ting, Eric

AU - Vezie, Michael

AU - Laughlin, Gregory

PY - 2019

Y1 - 2019

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 1.017+0.070/- 0.068 MJ and radius of 1.545 +0.052/-0.060 RJ, 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 1.017+0.070/- 0.068 MJ and radius of 1.545 +0.052/-0.060 RJ, 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

U2 - 10.3847/1538-3881/aaf1b7

DO - 10.3847/1538-3881/aaf1b7

M3 - Journal article

VL - 157

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 51

ER -