KELT-24b: A 5M J Planet on a 5.6 day Well-aligned Orbit around the Young V = 8.3 F-star HD 93148

We present the discovery of KELT-24 b, a massive hot Jupiter orbiting a bright ( V  = 8.3 mag, K  = 7.2 mag) young F-star with a period of 5.6 days. The host star, KELT-24 (HD 93148), has a T eff  =  K, a mass of M *  =  M ⊙ , a radius of R *  = 1.506 ± 0.022 R ⊙ , and an age of Gyr. Its planetary c...

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Veröffentlicht in:The Astronomical journal 2019-11, Vol.158 (5), p.197
Hauptverfasser: Rodriguez, Joseph E., Eastman, Jason D., Zhou, George, Quinn, Samuel N., Beatty, Thomas G., Penev, Kaloyan, Johnson, Marshall C., Cargile, Phillip A., Latham, David W., Bieryla, Allyson, Collins, Karen A., Dressing, Courtney D., Ciardi, David R., Relles, Howard M., Murawski, Gabriel, Nishiumi, Taku, Yonehara, Atsunori, Ishimaru, Ryo, Yoshida, Fumi, Gregorio, Joao, Lund, Michael B., Stevens, Daniel J., Stassun, Keivan G., Gaudi, B. Scott, Colón, Knicole D., Pepper, Joshua, Narita, Norio, Awiphan, Supachai, Chuanraksasat, Pongpichit, Benni, Paul, Zambelli, Roberto, Garrison, Lehman H., Wilson, Maurice L., Cornachione, Matthew A., Wang, Sharon X., Labadie-Bartz, Jonathan, Rodríguez, Romy, Siverd, Robert J., Yao, Xinyu, Bayliss, Daniel, Berlind, Perry, Calkins, Michael L., Christiansen, Jessie L., Cohen, David H., Conti, Dennis M., Curtis, Ivan A., Depoy, D. L., Esquerdo, Gilbert A., Evans, Phil, Feliz, Dax, Fulton, Benjamin J., Holoien, Thomas W.-S., James, David J., Jayasinghe, Tharindu, Jang-Condell, Hannah, Jensen, Eric L. N., Johnson, John A., Joner, Michael D., Khakpash, Somayeh, Kielkopf, John F., Kuhn, Rudolf B., Manner, Mark, Marshall, Jennifer L., McLeod, Kim K., McCrady, Nate, Oberst, Thomas E., Oelkers, Ryan J., Penny, Matthew T., Reed, Phillip A., Sliski, David H., Shappee, B. J., Stephens, Denise C., Stockdale, Chris, Tan, Thiam-Guan, Trueblood, Mark, Trueblood, Pat, Villanueva, Steven, Wittenmyer, Robert A., Wright, Jason T.
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container_issue 5
container_start_page 197
container_title The Astronomical journal
container_volume 158
creator Rodriguez, Joseph E.
Eastman, Jason D.
Zhou, George
Quinn, Samuel N.
Beatty, Thomas G.
Penev, Kaloyan
Johnson, Marshall C.
Cargile, Phillip A.
Latham, David W.
Bieryla, Allyson
Collins, Karen A.
Dressing, Courtney D.
Ciardi, David R.
Relles, Howard M.
Murawski, Gabriel
Nishiumi, Taku
Yonehara, Atsunori
Ishimaru, Ryo
Yoshida, Fumi
Gregorio, Joao
Lund, Michael B.
Stevens, Daniel J.
Stassun, Keivan G.
Gaudi, B. Scott
Colón, Knicole D.
Pepper, Joshua
Narita, Norio
Awiphan, Supachai
Chuanraksasat, Pongpichit
Benni, Paul
Zambelli, Roberto
Garrison, Lehman H.
Wilson, Maurice L.
Cornachione, Matthew A.
Wang, Sharon X.
Labadie-Bartz, Jonathan
Rodríguez, Romy
Siverd, Robert J.
Yao, Xinyu
Bayliss, Daniel
Berlind, Perry
Calkins, Michael L.
Christiansen, Jessie L.
Cohen, David H.
Conti, Dennis M.
Curtis, Ivan A.
Depoy, D. L.
Esquerdo, Gilbert A.
Evans, Phil
Feliz, Dax
Fulton, Benjamin J.
Holoien, Thomas W.-S.
James, David J.
Jayasinghe, Tharindu
Jang-Condell, Hannah
Jensen, Eric L. N.
Johnson, John A.
Joner, Michael D.
Khakpash, Somayeh
Kielkopf, John F.
Kuhn, Rudolf B.
Manner, Mark
Marshall, Jennifer L.
McLeod, Kim K.
McCrady, Nate
Oberst, Thomas E.
Oelkers, Ryan J.
Penny, Matthew T.
Reed, Phillip A.
Sliski, David H.
Shappee, B. J.
Stephens, Denise C.
Stockdale, Chris
Tan, Thiam-Guan
Trueblood, Mark
Trueblood, Pat
Villanueva, Steven
Wittenmyer, Robert A.
Wright, Jason T.
description We present the discovery of KELT-24 b, a massive hot Jupiter orbiting a bright ( V  = 8.3 mag, K  = 7.2 mag) young F-star with a period of 5.6 days. The host star, KELT-24 (HD 93148), has a T eff  =  K, a mass of M *  =  M ⊙ , a radius of R *  = 1.506 ± 0.022 R ⊙ , and an age of Gyr. Its planetary companion (KELT-24 b) has a radius of R P  = 1.272 ± 0.021 R J and a mass of M P  =  M J , and from Doppler tomographic observations, we find that the planet’s orbit is well-aligned to its host star’s projected spin axis ( ). The young age estimated for KELT-24 suggests that it only recently started to evolve from the zero-age main sequence. KELT-24 is the brightest star known to host a transiting giant planet with a period between 5 and 10 days. Although the circularization timescale is much longer than the age of the system, we do not detect a large eccentricity or significant misalignment that is expected from dynamical migration. The brightness of its host star and its moderate surface gravity make KELT-24b an intriguing target for detailed atmospheric characterization through spectroscopic emission measurements since it would bridge the current literature results that have primarily focused on lower mass hot Jupiters and a few brown dwarfs.
doi_str_mv 10.3847/1538-3881/ab4136
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Scott ; Colón, Knicole D. ; Pepper, Joshua ; Narita, Norio ; Awiphan, Supachai ; Chuanraksasat, Pongpichit ; Benni, Paul ; Zambelli, Roberto ; Garrison, Lehman H. ; Wilson, Maurice L. ; Cornachione, Matthew A. ; Wang, Sharon X. ; Labadie-Bartz, Jonathan ; Rodríguez, Romy ; Siverd, Robert J. ; Yao, Xinyu ; Bayliss, Daniel ; Berlind, Perry ; Calkins, Michael L. ; Christiansen, Jessie L. ; Cohen, David H. ; Conti, Dennis M. ; Curtis, Ivan A. ; Depoy, D. L. ; Esquerdo, Gilbert A. ; Evans, Phil ; Feliz, Dax ; Fulton, Benjamin J. ; Holoien, Thomas W.-S. ; James, David J. ; Jayasinghe, Tharindu ; Jang-Condell, Hannah ; Jensen, Eric L. N. ; Johnson, John A. ; Joner, Michael D. ; Khakpash, Somayeh ; Kielkopf, John F. ; Kuhn, Rudolf B. ; Manner, Mark ; Marshall, Jennifer L. ; McLeod, Kim K. ; McCrady, Nate ; Oberst, Thomas E. ; Oelkers, Ryan J. ; Penny, Matthew T. ; Reed, Phillip A. ; Sliski, David H. ; Shappee, B. 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Scott ; Colón, Knicole D. ; Pepper, Joshua ; Narita, Norio ; Awiphan, Supachai ; Chuanraksasat, Pongpichit ; Benni, Paul ; Zambelli, Roberto ; Garrison, Lehman H. ; Wilson, Maurice L. ; Cornachione, Matthew A. ; Wang, Sharon X. ; Labadie-Bartz, Jonathan ; Rodríguez, Romy ; Siverd, Robert J. ; Yao, Xinyu ; Bayliss, Daniel ; Berlind, Perry ; Calkins, Michael L. ; Christiansen, Jessie L. ; Cohen, David H. ; Conti, Dennis M. ; Curtis, Ivan A. ; Depoy, D. L. ; Esquerdo, Gilbert A. ; Evans, Phil ; Feliz, Dax ; Fulton, Benjamin J. ; Holoien, Thomas W.-S. ; James, David J. ; Jayasinghe, Tharindu ; Jang-Condell, Hannah ; Jensen, Eric L. N. ; Johnson, John A. ; Joner, Michael D. ; Khakpash, Somayeh ; Kielkopf, John F. ; Kuhn, Rudolf B. ; Manner, Mark ; Marshall, Jennifer L. ; McLeod, Kim K. ; McCrady, Nate ; Oberst, Thomas E. ; Oelkers, Ryan J. ; Penny, Matthew T. ; Reed, Phillip A. ; Sliski, David H. ; Shappee, B. 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Although the circularization timescale is much longer than the age of the system, we do not detect a large eccentricity or significant misalignment that is expected from dynamical migration. 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N.</creatorcontrib><creatorcontrib>Johnson, John A.</creatorcontrib><creatorcontrib>Joner, Michael D.</creatorcontrib><creatorcontrib>Khakpash, Somayeh</creatorcontrib><creatorcontrib>Kielkopf, John F.</creatorcontrib><creatorcontrib>Kuhn, Rudolf B.</creatorcontrib><creatorcontrib>Manner, Mark</creatorcontrib><creatorcontrib>Marshall, Jennifer L.</creatorcontrib><creatorcontrib>McLeod, Kim K.</creatorcontrib><creatorcontrib>McCrady, Nate</creatorcontrib><creatorcontrib>Oberst, Thomas E.</creatorcontrib><creatorcontrib>Oelkers, Ryan J.</creatorcontrib><creatorcontrib>Penny, Matthew T.</creatorcontrib><creatorcontrib>Reed, Phillip A.</creatorcontrib><creatorcontrib>Sliski, David H.</creatorcontrib><creatorcontrib>Shappee, B. J.</creatorcontrib><creatorcontrib>Stephens, Denise C.</creatorcontrib><creatorcontrib>Stockdale, Chris</creatorcontrib><creatorcontrib>Tan, Thiam-Guan</creatorcontrib><creatorcontrib>Trueblood, Mark</creatorcontrib><creatorcontrib>Trueblood, Pat</creatorcontrib><creatorcontrib>Villanueva, Steven</creatorcontrib><creatorcontrib>Wittenmyer, Robert A.</creatorcontrib><creatorcontrib>Wright, Jason T.</creatorcontrib><title>KELT-24b: A 5M J Planet on a 5.6 day Well-aligned Orbit around the Young V = 8.3 F-star HD 93148</title><title>The Astronomical journal</title><description>We present the discovery of KELT-24 b, a massive hot Jupiter orbiting a bright ( V  = 8.3 mag, K  = 7.2 mag) young F-star with a period of 5.6 days. The host star, KELT-24 (HD 93148), has a T eff  =  K, a mass of M *  =  M ⊙ , a radius of R *  = 1.506 ± 0.022 R ⊙ , and an age of Gyr. Its planetary companion (KELT-24 b) has a radius of R P  = 1.272 ± 0.021 R J and a mass of M P  =  M J , and from Doppler tomographic observations, we find that the planet’s orbit is well-aligned to its host star’s projected spin axis ( ). The young age estimated for KELT-24 suggests that it only recently started to evolve from the zero-age main sequence. KELT-24 is the brightest star known to host a transiting giant planet with a period between 5 and 10 days. Although the circularization timescale is much longer than the age of the system, we do not detect a large eccentricity or significant misalignment that is expected from dynamical migration. The brightness of its host star and its moderate surface gravity make KELT-24b an intriguing target for detailed atmospheric characterization through spectroscopic emission measurements since it would bridge the current literature results that have primarily focused on lower mass hot Jupiters and a few brown dwarfs.</description><issn>0004-6256</issn><issn>1538-3881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNo90MFOAjEUBdDGaCKie5fvBwrvta8zHRMXBEFUDC6IxtWkZTqIGQfTGRb8Dd_ClynBuLo3d3EXR4hrwp62nPbJaCu1tdR3nkknJ6LzP52KDiKyTJRJzsVF03wiElnkjvBPo-lcKvY3MADzDI_wUrk6tLCuwYHpJVC4LbyFqpKuWi3rUMAs-lULLq43dQHtR4D337aE1_3udr-zPQ1j2bQuwuQOMk1sL8VZ6aomXP1lV8zHo_lwIqez-4fhYCoX1iZSUcYZqbSwimwastQlVBoOXnvFJhAq9J6NNR6dsoVjJEbjTckmM46V7go83i7iumliKPPvuPpycZsT5gei_OCRHzzyI5H-AQLqVDg</recordid><startdate>20191101</startdate><enddate>20191101</enddate><creator>Rodriguez, Joseph E.</creator><creator>Eastman, Jason D.</creator><creator>Zhou, George</creator><creator>Quinn, Samuel N.</creator><creator>Beatty, Thomas G.</creator><creator>Penev, Kaloyan</creator><creator>Johnson, Marshall C.</creator><creator>Cargile, Phillip A.</creator><creator>Latham, David W.</creator><creator>Bieryla, Allyson</creator><creator>Collins, Karen A.</creator><creator>Dressing, Courtney D.</creator><creator>Ciardi, David R.</creator><creator>Relles, Howard M.</creator><creator>Murawski, Gabriel</creator><creator>Nishiumi, Taku</creator><creator>Yonehara, Atsunori</creator><creator>Ishimaru, Ryo</creator><creator>Yoshida, Fumi</creator><creator>Gregorio, Joao</creator><creator>Lund, Michael B.</creator><creator>Stevens, Daniel J.</creator><creator>Stassun, Keivan G.</creator><creator>Gaudi, B. 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Scott ; Colón, Knicole D. ; Pepper, Joshua ; Narita, Norio ; Awiphan, Supachai ; Chuanraksasat, Pongpichit ; Benni, Paul ; Zambelli, Roberto ; Garrison, Lehman H. ; Wilson, Maurice L. ; Cornachione, Matthew A. ; Wang, Sharon X. ; Labadie-Bartz, Jonathan ; Rodríguez, Romy ; Siverd, Robert J. ; Yao, Xinyu ; Bayliss, Daniel ; Berlind, Perry ; Calkins, Michael L. ; Christiansen, Jessie L. ; Cohen, David H. ; Conti, Dennis M. ; Curtis, Ivan A. ; Depoy, D. L. ; Esquerdo, Gilbert A. ; Evans, Phil ; Feliz, Dax ; Fulton, Benjamin J. ; Holoien, Thomas W.-S. ; James, David J. ; Jayasinghe, Tharindu ; Jang-Condell, Hannah ; Jensen, Eric L. N. ; Johnson, John A. ; Joner, Michael D. ; Khakpash, Somayeh ; Kielkopf, John F. ; Kuhn, Rudolf B. ; Manner, Mark ; Marshall, Jennifer L. ; McLeod, Kim K. ; McCrady, Nate ; Oberst, Thomas E. ; Oelkers, Ryan J. ; Penny, Matthew T. ; Reed, Phillip A. ; Sliski, David H. ; Shappee, B. J. ; Stephens, Denise C. ; Stockdale, Chris ; Tan, Thiam-Guan ; Trueblood, Mark ; Trueblood, Pat ; Villanueva, Steven ; Wittenmyer, Robert A. ; Wright, Jason T.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c886-21949127d82187e97a61f54eb3b245e1020bb4585b0a28da401405b5f4595a423</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Rodriguez, Joseph E.</creatorcontrib><creatorcontrib>Eastman, Jason D.</creatorcontrib><creatorcontrib>Zhou, George</creatorcontrib><creatorcontrib>Quinn, Samuel N.</creatorcontrib><creatorcontrib>Beatty, Thomas G.</creatorcontrib><creatorcontrib>Penev, Kaloyan</creatorcontrib><creatorcontrib>Johnson, Marshall C.</creatorcontrib><creatorcontrib>Cargile, Phillip A.</creatorcontrib><creatorcontrib>Latham, David W.</creatorcontrib><creatorcontrib>Bieryla, Allyson</creatorcontrib><creatorcontrib>Collins, Karen A.</creatorcontrib><creatorcontrib>Dressing, Courtney D.</creatorcontrib><creatorcontrib>Ciardi, David R.</creatorcontrib><creatorcontrib>Relles, Howard M.</creatorcontrib><creatorcontrib>Murawski, Gabriel</creatorcontrib><creatorcontrib>Nishiumi, Taku</creatorcontrib><creatorcontrib>Yonehara, Atsunori</creatorcontrib><creatorcontrib>Ishimaru, Ryo</creatorcontrib><creatorcontrib>Yoshida, Fumi</creatorcontrib><creatorcontrib>Gregorio, Joao</creatorcontrib><creatorcontrib>Lund, Michael B.</creatorcontrib><creatorcontrib>Stevens, Daniel J.</creatorcontrib><creatorcontrib>Stassun, Keivan G.</creatorcontrib><creatorcontrib>Gaudi, B. Scott</creatorcontrib><creatorcontrib>Colón, Knicole D.</creatorcontrib><creatorcontrib>Pepper, Joshua</creatorcontrib><creatorcontrib>Narita, Norio</creatorcontrib><creatorcontrib>Awiphan, Supachai</creatorcontrib><creatorcontrib>Chuanraksasat, Pongpichit</creatorcontrib><creatorcontrib>Benni, Paul</creatorcontrib><creatorcontrib>Zambelli, Roberto</creatorcontrib><creatorcontrib>Garrison, Lehman H.</creatorcontrib><creatorcontrib>Wilson, Maurice L.</creatorcontrib><creatorcontrib>Cornachione, Matthew A.</creatorcontrib><creatorcontrib>Wang, Sharon X.</creatorcontrib><creatorcontrib>Labadie-Bartz, Jonathan</creatorcontrib><creatorcontrib>Rodríguez, Romy</creatorcontrib><creatorcontrib>Siverd, Robert J.</creatorcontrib><creatorcontrib>Yao, Xinyu</creatorcontrib><creatorcontrib>Bayliss, Daniel</creatorcontrib><creatorcontrib>Berlind, Perry</creatorcontrib><creatorcontrib>Calkins, Michael L.</creatorcontrib><creatorcontrib>Christiansen, Jessie L.</creatorcontrib><creatorcontrib>Cohen, David H.</creatorcontrib><creatorcontrib>Conti, Dennis M.</creatorcontrib><creatorcontrib>Curtis, Ivan A.</creatorcontrib><creatorcontrib>Depoy, D. 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N.</creatorcontrib><creatorcontrib>Johnson, John A.</creatorcontrib><creatorcontrib>Joner, Michael D.</creatorcontrib><creatorcontrib>Khakpash, Somayeh</creatorcontrib><creatorcontrib>Kielkopf, John F.</creatorcontrib><creatorcontrib>Kuhn, Rudolf B.</creatorcontrib><creatorcontrib>Manner, Mark</creatorcontrib><creatorcontrib>Marshall, Jennifer L.</creatorcontrib><creatorcontrib>McLeod, Kim K.</creatorcontrib><creatorcontrib>McCrady, Nate</creatorcontrib><creatorcontrib>Oberst, Thomas E.</creatorcontrib><creatorcontrib>Oelkers, Ryan J.</creatorcontrib><creatorcontrib>Penny, Matthew T.</creatorcontrib><creatorcontrib>Reed, Phillip A.</creatorcontrib><creatorcontrib>Sliski, David H.</creatorcontrib><creatorcontrib>Shappee, B. J.</creatorcontrib><creatorcontrib>Stephens, Denise C.</creatorcontrib><creatorcontrib>Stockdale, Chris</creatorcontrib><creatorcontrib>Tan, Thiam-Guan</creatorcontrib><creatorcontrib>Trueblood, Mark</creatorcontrib><creatorcontrib>Trueblood, Pat</creatorcontrib><creatorcontrib>Villanueva, Steven</creatorcontrib><creatorcontrib>Wittenmyer, Robert A.</creatorcontrib><creatorcontrib>Wright, Jason T.</creatorcontrib><collection>CrossRef</collection><jtitle>The Astronomical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Rodriguez, Joseph E.</au><au>Eastman, Jason D.</au><au>Zhou, George</au><au>Quinn, Samuel N.</au><au>Beatty, Thomas G.</au><au>Penev, Kaloyan</au><au>Johnson, Marshall C.</au><au>Cargile, Phillip A.</au><au>Latham, David W.</au><au>Bieryla, Allyson</au><au>Collins, Karen A.</au><au>Dressing, Courtney D.</au><au>Ciardi, David R.</au><au>Relles, Howard M.</au><au>Murawski, Gabriel</au><au>Nishiumi, Taku</au><au>Yonehara, Atsunori</au><au>Ishimaru, Ryo</au><au>Yoshida, Fumi</au><au>Gregorio, Joao</au><au>Lund, Michael B.</au><au>Stevens, Daniel J.</au><au>Stassun, Keivan G.</au><au>Gaudi, B. Scott</au><au>Colón, Knicole D.</au><au>Pepper, Joshua</au><au>Narita, Norio</au><au>Awiphan, Supachai</au><au>Chuanraksasat, Pongpichit</au><au>Benni, Paul</au><au>Zambelli, Roberto</au><au>Garrison, Lehman H.</au><au>Wilson, Maurice L.</au><au>Cornachione, Matthew A.</au><au>Wang, Sharon X.</au><au>Labadie-Bartz, Jonathan</au><au>Rodríguez, Romy</au><au>Siverd, Robert J.</au><au>Yao, Xinyu</au><au>Bayliss, Daniel</au><au>Berlind, Perry</au><au>Calkins, Michael L.</au><au>Christiansen, Jessie L.</au><au>Cohen, David H.</au><au>Conti, Dennis M.</au><au>Curtis, Ivan A.</au><au>Depoy, D. L.</au><au>Esquerdo, Gilbert A.</au><au>Evans, Phil</au><au>Feliz, Dax</au><au>Fulton, Benjamin J.</au><au>Holoien, Thomas W.-S.</au><au>James, David J.</au><au>Jayasinghe, Tharindu</au><au>Jang-Condell, Hannah</au><au>Jensen, Eric L. N.</au><au>Johnson, John A.</au><au>Joner, Michael D.</au><au>Khakpash, Somayeh</au><au>Kielkopf, John F.</au><au>Kuhn, Rudolf B.</au><au>Manner, Mark</au><au>Marshall, Jennifer L.</au><au>McLeod, Kim K.</au><au>McCrady, Nate</au><au>Oberst, Thomas E.</au><au>Oelkers, Ryan J.</au><au>Penny, Matthew T.</au><au>Reed, Phillip A.</au><au>Sliski, David H.</au><au>Shappee, B. J.</au><au>Stephens, Denise C.</au><au>Stockdale, Chris</au><au>Tan, Thiam-Guan</au><au>Trueblood, Mark</au><au>Trueblood, Pat</au><au>Villanueva, Steven</au><au>Wittenmyer, Robert A.</au><au>Wright, Jason T.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>KELT-24b: A 5M J Planet on a 5.6 day Well-aligned Orbit around the Young V = 8.3 F-star HD 93148</atitle><jtitle>The Astronomical journal</jtitle><date>2019-11-01</date><risdate>2019</risdate><volume>158</volume><issue>5</issue><spage>197</spage><pages>197-</pages><issn>0004-6256</issn><eissn>1538-3881</eissn><abstract>We present the discovery of KELT-24 b, a massive hot Jupiter orbiting a bright ( V  = 8.3 mag, K  = 7.2 mag) young F-star with a period of 5.6 days. The host star, KELT-24 (HD 93148), has a T eff  =  K, a mass of M *  =  M ⊙ , a radius of R *  = 1.506 ± 0.022 R ⊙ , and an age of Gyr. Its planetary companion (KELT-24 b) has a radius of R P  = 1.272 ± 0.021 R J and a mass of M P  =  M J , and from Doppler tomographic observations, we find that the planet’s orbit is well-aligned to its host star’s projected spin axis ( ). The young age estimated for KELT-24 suggests that it only recently started to evolve from the zero-age main sequence. KELT-24 is the brightest star known to host a transiting giant planet with a period between 5 and 10 days. Although the circularization timescale is much longer than the age of the system, we do not detect a large eccentricity or significant misalignment that is expected from dynamical migration. The brightness of its host star and its moderate surface gravity make KELT-24b an intriguing target for detailed atmospheric characterization through spectroscopic emission measurements since it would bridge the current literature results that have primarily focused on lower mass hot Jupiters and a few brown dwarfs.</abstract><doi>10.3847/1538-3881/ab4136</doi><orcidid>https://orcid.org/0000-0002-1910-7065</orcidid><orcidid>https://orcid.org/0000-0003-2163-1437</orcidid><orcidid>https://orcid.org/0000-0003-2527-1598</orcidid><orcidid>https://orcid.org/0000-0002-9853-5673</orcidid><orcidid>https://orcid.org/0000-0001-9206-3460</orcidid><orcidid>https://orcid.org/0000-0002-2457-7889</orcidid><orcidid>https://orcid.org/0000-0002-8964-8377</orcidid><orcidid>https://orcid.org/0000-0001-5160-4486</orcidid><orcidid>https://orcid.org/0000-0001-6213-8804</orcidid><orcidid>https://orcid.org/0000-0002-2830-5661</orcidid><orcidid>https://orcid.org/0000-0003-3773-5142</orcidid><orcidid>https://orcid.org/0000-0001-6160-5888</orcidid><orcidid>https://orcid.org/0000-0002-3481-9052</orcidid><orcidid>https://orcid.org/0000-0001-6588-9574</orcidid><orcidid>https://orcid.org/0000-0001-5603-6895</orcidid><orcidid>https://orcid.org/0000-0001-8189-0233</orcidid><orcidid>https://orcid.org/0000-0002-5951-8328</orcidid><orcidid>https://orcid.org/0000-0003-0395-9869</orcidid><orcidid>https://orcid.org/0000-0003-4631-1149</orcidid><orcidid>https://orcid.org/0000-0001-9957-9304</orcidid><orcidid>https://orcid.org/0000-0001-8812-0565</orcidid><orcidid>https://orcid.org/0000-0002-4625-7333</orcidid><orcidid>https://orcid.org/0000-0003-0710-9474</orcidid><orcidid>https://orcid.org/0000-0002-5005-1215</orcidid><orcidid>https://orcid.org/0000-0002-4891-3517</orcidid><orcidid>https://orcid.org/0000-0003-4464-1371</orcidid><orcidid>https://orcid.org/0000-0002-2919-6786</orcidid><orcidid>https://orcid.org/0000-0002-9539-4203</orcidid><orcidid>https://orcid.org/0000-0003-1012-4771</orcidid><orcidid>https://orcid.org/0000-0002-3286-911X</orcidid><orcidid>https://orcid.org/0000-0002-5099-8185</orcidid><orcidid>https://orcid.org/0000-0001-6023-1335</orcidid><orcidid>https://orcid.org/0000-0002-6244-477X</orcidid><orcidid>https://orcid.org/0000-0002-9411-7271</orcidid><orcidid>https://orcid.org/0000-0001-9911-7388</orcidid><orcidid>https://orcid.org/0000-0001-8020-7121</orcidid><orcidid>https://orcid.org/0000-0002-0582-1751</orcidid><orcidid>https://orcid.org/0000-0002-7639-1322</orcidid><orcidid>https://orcid.org/0000-0002-8035-4778</orcidid><orcidid>https://orcid.org/0000-0001-6637-5401</orcidid><orcidid>https://orcid.org/0000-0001-8511-2981</orcidid><orcidid>https://orcid.org/0000-0002-3827-8417</orcidid><orcidid>https://orcid.org/0000-0003-4554-5592</orcidid><orcidid>https://orcid.org/0000-0003-3504-5316</orcidid><orcidid>https://orcid.org/0000-0001-7506-5640</orcidid><orcidid>https://orcid.org/0000-0001-9504-1486</orcidid></addata></record>
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title KELT-24b: A 5M J Planet on a 5.6 day Well-aligned Orbit around the Young V = 8.3 F-star HD 93148
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