Migration and Evolution of giant ExoPlanets (MEEP). I. Nine newly confirmed hot Jupiters from the TESS mission

Jack Schulte; Joseph E. Rodriguez; Allyson Bieryla; Samuel N. Quinn; Karen A. Collins; Samuel W. Yee; Andrew C. Nine; Melinda Soares-Furtado; David W. Latham; Jason D. Eastman; Khalid Barkaoui; David R. Ciardi; Diana Dragomir; Mark E. Everett; Steven Giacalone; Ismael Mireles; Felipe Murgas; Norio Narita; Avi Shporer; Ivan A. Strakhov; Stephanie Striegel; Martin Vaňko; Noah Vowell; Gavin Wang; Carl Ziegler; Michael Bellaver; Paul Benni; Serge Bergeron; Henri M. J. Boffin; César Briceño; Catherine A. Clark; Kevin I. Collins; Jerome P. de Leon; Courtney D. Dressing; Phil Evans; Emma Esparza-Borges; Jeremy Fedewa; Akihiko Fukui; Tianjun Gan; Ivan S. Gerasimov; Joel D. Hartman; Holden Gill; Michaël Gillon; Keith Horne; Ferran Grau Horta; Steve B. Howell; Keisuke Isogai; Emmanuël Jehin; Jon M. Jenkins; Raine Karjalainen; John F. Kielkopf; Kathryn V. Lester; Colin Littlefield; Michael B. Lund; Andrew W. Mann; Mason McCormack; Edward J. Michaels; Shane Painter; Enric Palle; Hannu Parviainen; David-Michael Peterson; Francisco J. Pozuelos; Zachary Raup; Phillip Reed; Howard M. Relles; George R. Ricker; Arjun B. Savel; Richard P. Schwarz; S. Seager; Ramotholo Sefako; Gregor Srdoc; Chris Stockdale; Hannah Sullivan; Mathilde Timmermans; Joshua N. Winn

doi:10.3847/1538-3881/ad4a57

Migration and Evolution of giant ExoPlanets (MEEP). I. Nine newly confirmed hot Jupiters from the TESS mission

Jack Schulte^*, Joseph E. Rodriguez, Allyson Bieryla, Samuel N. Quinn, Karen A. Collins, Samuel W. Yee, Andrew C. Nine, Melinda Soares-Furtado, David W. Latham, Jason D. Eastman, Khalid Barkaoui, David R. Ciardi, Diana Dragomir, Mark E. Everett, Steven Giacalone, Ismael Mireles, Felipe Murgas, Norio Narita, Avi Shporer, Ivan A. StrakhovStephanie Striegel, Martin Vaňko, Noah Vowell, Gavin Wang, Carl Ziegler, Michael Bellaver, Paul Benni, Serge Bergeron, Henri M. J. Boffin, César Briceño, Catherine A. Clark, Kevin I. Collins, Jerome P. de Leon, Courtney D. Dressing, Phil Evans, Emma Esparza-Borges, Jeremy Fedewa, Akihiko Fukui, Tianjun Gan, Ivan S. Gerasimov, Joel D. Hartman, Holden Gill, Michaël Gillon, Keith Horne, Ferran Grau Horta, Steve B. Howell, Keisuke Isogai, Emmanuël Jehin, Jon M. Jenkins, Raine Karjalainen, John F. Kielkopf, Kathryn V. Lester, Colin Littlefield, Michael B. Lund, Andrew W. Mann, Mason McCormack, Edward J. Michaels, Shane Painter, Enric Palle, Hannu Parviainen, David-Michael Peterson, Francisco J. Pozuelos, Zachary Raup, Phillip Reed, Howard M. Relles, George R. Ricker, Arjun B. Savel, Richard P. Schwarz, S. Seager, Ramotholo Sefako, Gregor Srdoc, Chris Stockdale, Hannah Sullivan, Mathilde Timmermans, Joshua N. Winn

^*Corresponding author for this work

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

Abstract

Hot Jupiters were many of the first exoplanets discovered in the 1990s, but in the decades since their discovery the mysteries surrounding their origins have remained. Here we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b, TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-4153 b, TOI-5232 b, and TOI-5301 b) discovered by NASA’s TESS mission and confirmed using ground-based imaging and spectroscopy. These discoveries are the first in a series of papers named the Migration and Evolution of giant ExoPlanets survey and are part of an ongoing effort to build a complete sample of hot Jupiters orbiting FGK stars, with a limiting Gaia G-band magnitude of 12.5. This effort aims to use homogeneous detection and analysis techniques to generate a set of precisely measured stellar and planetary properties that is ripe for statistical analysis. The nine planets presented in this work occupy a range of masses (0.55M _J < M_P < 3.88M _J) and sizes (0.967R _J < R_P < 1.438R _J) and orbit stars that have an effective temperature in the range of 5360 K < T_eff< 6860 K with Gaia G-band magnitudes ranging from 11.1 to 12.7. Two of the planets in our sample have detectable orbital eccentricity: TOI-3919 b (e = 0.259_−0.036^+0.033) and TOI-5301 b (e = 0.33_−0.10^+0.11). These eccentric planets join a growing sample of eccentric hot Jupiters that are consistent with high-eccentricity tidal migration, one of the three most prominent theories explaining hot Jupiter formation and evolution.

Original language	English
Article number	32
Number of pages	30
Journal	Astronomical Journal
Volume	168
Issue number	1
Early online date	25 Jun 2024
DOIs	https://doi.org/10.3847/1538-3881/ad4a57
Publication status	Published - 1 Jul 2024

Keywords

Exoplanets
Direct imaging
Exoplanet astronomy
Radial velocity
Exoplanet migration
Transits
Exoplanet detection methods

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Schulte, J., Rodriguez, J. E., Bieryla, A., Quinn, S. N., Collins, K. A., Yee, S. W., Nine, A. C., Soares-Furtado, M., Latham, D. W., Eastman, J. D., Barkaoui, K., Ciardi, D. R., Dragomir, D., Everett, M. E., Giacalone, S., Mireles, I., Murgas, F., Narita, N., Shporer, A., ... Winn, J. N. (2024). Migration and Evolution of giant ExoPlanets (MEEP). I. Nine newly confirmed hot Jupiters from the TESS mission. Astronomical Journal, 168(1), Article 32. https://doi.org/10.3847/1538-3881/ad4a57

@article{8f0080a17b3d4a389101ad910501e1c4,

title = "Migration and Evolution of giant ExoPlanets (MEEP). I. Nine newly confirmed hot Jupiters from the TESS mission",

abstract = "Hot Jupiters were many of the first exoplanets discovered in the 1990s, but in the decades since their discovery the mysteries surrounding their origins have remained. Here we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b, TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-4153 b, TOI-5232 b, and TOI-5301 b) discovered by NASA{\textquoteright}s TESS mission and confirmed using ground-based imaging and spectroscopy. These discoveries are the first in a series of papers named the Migration and Evolution of giant ExoPlanets survey and are part of an ongoing effort to build a complete sample of hot Jupiters orbiting FGK stars, with a limiting Gaia G-band magnitude of 12.5. This effort aims to use homogeneous detection and analysis techniques to generate a set of precisely measured stellar and planetary properties that is ripe for statistical analysis. The nine planets presented in this work occupy a range of masses (0.55M J < MP < 3.88M J) and sizes (0.967R J < RP < 1.438R J) and orbit stars that have an effective temperature in the range of 5360 K < Teff < 6860 K with Gaia G-band magnitudes ranging from 11.1 to 12.7. Two of the planets in our sample have detectable orbital eccentricity: TOI-3919 b (e = 0.259−0.036+0.033) and TOI-5301 b (e = 0.33−0.10+0.11). These eccentric planets join a growing sample of eccentric hot Jupiters that are consistent with high-eccentricity tidal migration, one of the three most prominent theories explaining hot Jupiter formation and evolution.",

keywords = "Exoplanets, Direct imaging, Exoplanet astronomy, Radial velocity, Exoplanet migration, Transits, Exoplanet detection methods",

author = "Jack Schulte and Rodriguez, {Joseph E.} and Allyson Bieryla and Quinn, {Samuel N.} and Collins, {Karen A.} and Yee, {Samuel W.} and Nine, {Andrew C.} and Melinda Soares-Furtado and Latham, {David W.} and Eastman, {Jason D.} and Khalid Barkaoui and Ciardi, {David R.} and Diana Dragomir and Everett, {Mark E.} and Steven Giacalone and Ismael Mireles and Felipe Murgas and Norio Narita and Avi Shporer and Strakhov, {Ivan A.} and Stephanie Striegel and Martin Va{\v n}ko and Noah Vowell and Gavin Wang and Carl Ziegler and Michael Bellaver and Paul Benni and Serge Bergeron and Boffin, {Henri M. J.} and C{\'e}sar Brice{\~n}o and Clark, {Catherine A.} and Collins, {Kevin I.} and {de Leon}, {Jerome P.} and Dressing, {Courtney D.} and Phil Evans and Emma Esparza-Borges and Jeremy Fedewa and Akihiko Fukui and Tianjun Gan and Gerasimov, {Ivan S.} and Hartman, {Joel D.} and Holden Gill and Micha{\"e}l Gillon and Keith Horne and {Grau Horta}, Ferran and Howell, {Steve B.} and Keisuke Isogai and Emmanu{\"e}l Jehin and Jenkins, {Jon M.} and Raine Karjalainen and Kielkopf, {John F.} and Lester, {Kathryn V.} and Colin Littlefield and Lund, {Michael B.} and Mann, {Andrew W.} and Mason McCormack and Michaels, {Edward J.} and Shane Painter and Enric Palle and Hannu Parviainen and David-Michael Peterson and Pozuelos, {Francisco J.} and Zachary Raup and Phillip Reed and Relles, {Howard M.} and Ricker, {George R.} and Savel, {Arjun B.} and Schwarz, {Richard P.} and S. Seager and Ramotholo Sefako and Gregor Srdoc and Chris Stockdale and Hannah Sullivan and Mathilde Timmermans and Winn, {Joshua N.}",

note = "Funding: E.P. acknowledges funding from the Spanish Ministry of Economics and Competitiveness through project PGC2021-125627OB-C32. TRAPPIST-South is funded by the Belgian National Fund for Scientific Research (F.R.S.-FNRS) under grant PDR T.0120.21, with the participation of the Swiss National Science Fundation (SNF). M.G. and E.J. are FNRS Senior Research Associates. The postdoctoral fellowship of K.B. is funded by F.R.S.-FNRS grant T.0109.20 and by the Francqui Foundation. This work is partly supported by JSPS KAKENHI grant Nos. JP17H04574, JP18H05439, JP20K14521, and JP21K13955 and JST CREST grant No. JPMJCR1761. The research of M.V. was supported by the Slovak Research and Development Agency, under contract No. APVV-20-0148. This publication benefits from the support of the French Community of Belgium in the context of the FRIA doctoral grant awarded to M.T. We acknowledge financial support from the Agencia Estatal de Investigaci{\'o}n of the Ministerio de Ciencia e Innovaci{\'o}n MCIN/AEI/10.13039/501100011033 and the ERDF {"}A way of making Europe{"} through project PID2021-125627OB-C32, and from the Centre of Excellence {"}Severo Ochoa{"} award to the Instituto de Astrofisica de Canarias. P.A.R. acknowledges support from the National Science Foundation under grant No. 1952545. R.K. acknowledges the support by Inter-transfer grant No. LTT-20015. F.J.P. acknowledges financial support from the grant CEX2021-001131-S funded by MCIN/AEI/ 10.13039/501100011033 and through projects PID2019-109522GB-C52 and PID2022-137241NB-C43. H.P. acknowledges support by the Spanish Ministry of Science and Innovation with the Ramon y Cajal fellowship No. RYC2021-031798-I. C.A.C. acknowledges that this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004). ",

year = "2024",

month = jul,

day = "1",

doi = "10.3847/1538-3881/ad4a57",

language = "English",

volume = "168",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

number = "1",

}

Schulte, J, Rodriguez, JE, Bieryla, A, Quinn, SN, Collins, KA, Yee, SW, Nine, AC, Soares-Furtado, M, Latham, DW, Eastman, JD, Barkaoui, K, Ciardi, DR, Dragomir, D, Everett, ME, Giacalone, S, Mireles, I, Murgas, F, Narita, N, Shporer, A, Strakhov, IA, Striegel, S, Vaňko, M, Vowell, N, Wang, G, Ziegler, C, Bellaver, M, Benni, P, Bergeron, S, Boffin, HMJ, Briceño, C, Clark, CA, Collins, KI, de Leon, JP, Dressing, CD, Evans, P, Esparza-Borges, E, Fedewa, J, Fukui, A, Gan, T, Gerasimov, IS, Hartman, JD, Gill, H, Gillon, M, Horne, K, Grau Horta, F, Howell, SB, Isogai, K, Jehin, E, Jenkins, JM, Karjalainen, R, Kielkopf, JF, Lester, KV, Littlefield, C, Lund, MB, Mann, AW, McCormack, M, Michaels, EJ, Painter, S, Palle, E, Parviainen, H, Peterson, D-M, Pozuelos, FJ, Raup, Z, Reed, P, Relles, HM, Ricker, GR, Savel, AB, Schwarz, RP, Seager, S, Sefako, R, Srdoc, G, Stockdale, C, Sullivan, H, Timmermans, M & Winn, JN 2024, 'Migration and Evolution of giant ExoPlanets (MEEP). I. Nine newly confirmed hot Jupiters from the TESS mission', Astronomical Journal, vol. 168, no. 1, 32. https://doi.org/10.3847/1538-3881/ad4a57

TY - JOUR

T1 - Migration and Evolution of giant ExoPlanets (MEEP). I. Nine newly confirmed hot Jupiters from the TESS mission

AU - Schulte, Jack

AU - Rodriguez, Joseph E.

AU - Bieryla, Allyson

AU - Quinn, Samuel N.

AU - Collins, Karen A.

AU - Yee, Samuel W.

AU - Nine, Andrew C.

AU - Soares-Furtado, Melinda

AU - Latham, David W.

AU - Eastman, Jason D.

AU - Barkaoui, Khalid

AU - Ciardi, David R.

AU - Dragomir, Diana

AU - Everett, Mark E.

AU - Giacalone, Steven

AU - Mireles, Ismael

AU - Murgas, Felipe

AU - Narita, Norio

AU - Shporer, Avi

AU - Strakhov, Ivan A.

AU - Striegel, Stephanie

AU - Vaňko, Martin

AU - Vowell, Noah

AU - Wang, Gavin

AU - Ziegler, Carl

AU - Bellaver, Michael

AU - Benni, Paul

AU - Bergeron, Serge

AU - Boffin, Henri M. J.

AU - Briceño, César

AU - Clark, Catherine A.

AU - Collins, Kevin I.

AU - de Leon, Jerome P.

AU - Dressing, Courtney D.

AU - Evans, Phil

AU - Esparza-Borges, Emma

AU - Fedewa, Jeremy

AU - Fukui, Akihiko

AU - Gan, Tianjun

AU - Gerasimov, Ivan S.

AU - Hartman, Joel D.

AU - Gill, Holden

AU - Gillon, Michaël

AU - Horne, Keith

AU - Grau Horta, Ferran

AU - Howell, Steve B.

AU - Isogai, Keisuke

AU - Jehin, Emmanuël

AU - Jenkins, Jon M.

AU - Karjalainen, Raine

AU - Kielkopf, John F.

AU - Lester, Kathryn V.

AU - Littlefield, Colin

AU - Lund, Michael B.

AU - Mann, Andrew W.

AU - McCormack, Mason

AU - Michaels, Edward J.

AU - Painter, Shane

AU - Palle, Enric

AU - Parviainen, Hannu

AU - Peterson, David-Michael

AU - Pozuelos, Francisco J.

AU - Raup, Zachary

AU - Reed, Phillip

AU - Relles, Howard M.

AU - Ricker, George R.

AU - Savel, Arjun B.

AU - Schwarz, Richard P.

AU - Seager, S.

AU - Sefako, Ramotholo

AU - Srdoc, Gregor

AU - Stockdale, Chris

AU - Sullivan, Hannah

AU - Timmermans, Mathilde

AU - Winn, Joshua N.

N1 - Funding: E.P. acknowledges funding from the Spanish Ministry of Economics and Competitiveness through project PGC2021-125627OB-C32. TRAPPIST-South is funded by the Belgian National Fund for Scientific Research (F.R.S.-FNRS) under grant PDR T.0120.21, with the participation of the Swiss National Science Fundation (SNF). M.G. and E.J. are FNRS Senior Research Associates. The postdoctoral fellowship of K.B. is funded by F.R.S.-FNRS grant T.0109.20 and by the Francqui Foundation. This work is partly supported by JSPS KAKENHI grant Nos. JP17H04574, JP18H05439, JP20K14521, and JP21K13955 and JST CREST grant No. JPMJCR1761. The research of M.V. was supported by the Slovak Research and Development Agency, under contract No. APVV-20-0148. This publication benefits from the support of the French Community of Belgium in the context of the FRIA doctoral grant awarded to M.T. We acknowledge financial support from the Agencia Estatal de Investigación of the Ministerio de Ciencia e Innovación MCIN/AEI/10.13039/501100011033 and the ERDF "A way of making Europe" through project PID2021-125627OB-C32, and from the Centre of Excellence "Severo Ochoa" award to the Instituto de Astrofisica de Canarias. P.A.R. acknowledges support from the National Science Foundation under grant No. 1952545. R.K. acknowledges the support by Inter-transfer grant No. LTT-20015. F.J.P. acknowledges financial support from the grant CEX2021-001131-S funded by MCIN/AEI/ 10.13039/501100011033 and through projects PID2019-109522GB-C52 and PID2022-137241NB-C43. H.P. acknowledges support by the Spanish Ministry of Science and Innovation with the Ramon y Cajal fellowship No. RYC2021-031798-I. C.A.C. acknowledges that this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004).

PY - 2024/7/1

Y1 - 2024/7/1

N2 - Hot Jupiters were many of the first exoplanets discovered in the 1990s, but in the decades since their discovery the mysteries surrounding their origins have remained. Here we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b, TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-4153 b, TOI-5232 b, and TOI-5301 b) discovered by NASA’s TESS mission and confirmed using ground-based imaging and spectroscopy. These discoveries are the first in a series of papers named the Migration and Evolution of giant ExoPlanets survey and are part of an ongoing effort to build a complete sample of hot Jupiters orbiting FGK stars, with a limiting Gaia G-band magnitude of 12.5. This effort aims to use homogeneous detection and analysis techniques to generate a set of precisely measured stellar and planetary properties that is ripe for statistical analysis. The nine planets presented in this work occupy a range of masses (0.55M J < MP < 3.88M J) and sizes (0.967R J < RP < 1.438R J) and orbit stars that have an effective temperature in the range of 5360 K < Teff < 6860 K with Gaia G-band magnitudes ranging from 11.1 to 12.7. Two of the planets in our sample have detectable orbital eccentricity: TOI-3919 b (e = 0.259−0.036+0.033) and TOI-5301 b (e = 0.33−0.10+0.11). These eccentric planets join a growing sample of eccentric hot Jupiters that are consistent with high-eccentricity tidal migration, one of the three most prominent theories explaining hot Jupiter formation and evolution.

AB - Hot Jupiters were many of the first exoplanets discovered in the 1990s, but in the decades since their discovery the mysteries surrounding their origins have remained. Here we present nine new hot Jupiters (TOI-1855 b, TOI-2107 b, TOI-2368 b, TOI-3321 b, TOI-3894 b, TOI-3919 b, TOI-4153 b, TOI-5232 b, and TOI-5301 b) discovered by NASA’s TESS mission and confirmed using ground-based imaging and spectroscopy. These discoveries are the first in a series of papers named the Migration and Evolution of giant ExoPlanets survey and are part of an ongoing effort to build a complete sample of hot Jupiters orbiting FGK stars, with a limiting Gaia G-band magnitude of 12.5. This effort aims to use homogeneous detection and analysis techniques to generate a set of precisely measured stellar and planetary properties that is ripe for statistical analysis. The nine planets presented in this work occupy a range of masses (0.55M J < MP < 3.88M J) and sizes (0.967R J < RP < 1.438R J) and orbit stars that have an effective temperature in the range of 5360 K < Teff < 6860 K with Gaia G-band magnitudes ranging from 11.1 to 12.7. Two of the planets in our sample have detectable orbital eccentricity: TOI-3919 b (e = 0.259−0.036+0.033) and TOI-5301 b (e = 0.33−0.10+0.11). These eccentric planets join a growing sample of eccentric hot Jupiters that are consistent with high-eccentricity tidal migration, one of the three most prominent theories explaining hot Jupiter formation and evolution.

KW - Exoplanets

KW - Direct imaging

KW - Exoplanet astronomy

KW - Radial velocity

KW - Exoplanet migration

KW - Transits

KW - Exoplanet detection methods

U2 - 10.3847/1538-3881/ad4a57

DO - 10.3847/1538-3881/ad4a57

M3 - Article

SN - 0004-6256

VL - 168

JO - Astronomical Journal

JF - Astronomical Journal

IS - 1

M1 - 32

ER -

Migration and Evolution of giant ExoPlanets (MEEP). I. Nine newly confirmed hot Jupiters from the TESS mission

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