TOI-3984 A b and TOI-5293 A b: two temperate gas giants transiting mid-M dwarfs in wide binary systems
We confirm the planetary nature of two gas giants discovered by TESS to transit M dwarfs with stellar companions at wide separations. TOI-3984 A (\(J=11.93\)) is an M4 dwarf hosting a short-period (\(4.353326 \pm 0.000005\) days) gas giant (\(M_p=0.14\pm0.03~\mathrm{M_{J}}\) and \(R_p=0.71\pm0.02~\m...
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| creator | Cañas, Caleb I Kanodia, Shubham Libby-Roberts, Jessica Lin, Andrea S J Schutte, Maria Powers, Luke Jones, Sinclaire Monson, Andrew Wang, Songhu Stefánsson, Guðmundur Cochran, William D Robertson, Paul Mahadevan, Suvrath Kowalski, Adam F Wisniewski, John Parker, Brock A Larsen, Alexander Chapman, Franklin A L Kobulnicky, Henry A Gupta, Arvind F Everett, Mark E Penprase, Bryan Edward Zeimann, Gregory Beard, Corey Bender, Chad F Colón, Knicole D Diddams, Scott A Connor, Fredrick Halverson, Samuel Ninan, Joe P Ramsey, Lawrence W Roy, Arpita Schwab, Christian |
| description | We confirm the planetary nature of two gas giants discovered by TESS to transit M dwarfs with stellar companions at wide separations. TOI-3984 A (\(J=11.93\)) is an M4 dwarf hosting a short-period (\(4.353326 \pm 0.000005\) days) gas giant (\(M_p=0.14\pm0.03~\mathrm{M_{J}}\) and \(R_p=0.71\pm0.02~\mathrm{R_{J}}\)) with a wide separation white dwarf companion. TOI-5293 A (\(J=12.47\)) is an M3 dwarf hosting a short-period (\(2.930289 \pm 0.000004\) days) gas giant (\(M_p=0.54\pm0.07~\mathrm{M_{J}}\) and \(R_p=1.06\pm0.04~\mathrm{R_{J}}\)) with a wide separation M dwarf companion. We characterize both systems using a combination of ground-based and space-based photometry, speckle imaging, and high-precision radial velocities from the Habitable-zone Planet Finder and NEID spectrographs. TOI-3984 A b (\(T_{eq}=563\pm15\) K and \(\mathrm{TSM}=138_{-27}^{+29}\)) and TOI-5293 A b (\(T_{eq}=675_{-30}^{+42}\) K and \(\mathrm{TSM}=92\pm14\)) are two of the coolest gas giants among the population of hot Jupiter-sized gas planets orbiting M dwarfs and are favorable targets for atmospheric characterization of temperate gas giants and three-dimensional obliquity measurements to probe system architecture and migration scenarios. |
| doi_str_mv | 10.48550/arxiv.2302.07714 |
| format | Article |
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TOI-3984 A (\(J=11.93\)) is an M4 dwarf hosting a short-period (\(4.353326 \pm 0.000005\) days) gas giant (\(M_p=0.14\pm0.03~\mathrm{M_{J}}\) and \(R_p=0.71\pm0.02~\mathrm{R_{J}}\)) with a wide separation white dwarf companion. TOI-5293 A (\(J=12.47\)) is an M3 dwarf hosting a short-period (\(2.930289 \pm 0.000004\) days) gas giant (\(M_p=0.54\pm0.07~\mathrm{M_{J}}\) and \(R_p=1.06\pm0.04~\mathrm{R_{J}}\)) with a wide separation M dwarf companion. We characterize both systems using a combination of ground-based and space-based photometry, speckle imaging, and high-precision radial velocities from the Habitable-zone Planet Finder and NEID spectrographs. TOI-3984 A b (\(T_{eq}=563\pm15\) K and \(\mathrm{TSM}=138_{-27}^{+29}\)) and TOI-5293 A b (\(T_{eq}=675_{-30}^{+42}\) K and \(\mathrm{TSM}=92\pm14\)) are two of the coolest gas giants among the population of hot Jupiter-sized gas planets orbiting M dwarfs and are favorable targets for atmospheric characterization of temperate gas giants and three-dimensional obliquity measurements to probe system architecture and migration scenarios.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2302.07714</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Binary stars ; Circumstellar habitable zone ; Computer architecture ; Extrasolar planets ; Gas giant planets ; Jupiter ; Physics - Earth and Planetary Astrophysics ; Physics - Solar and Stellar Astrophysics ; Red dwarf stars ; Separation ; Spectrographs ; White dwarf stars</subject><ispartof>arXiv.org, 2023-06</ispartof><rights>2023. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,784,885,27925</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.2302.07714$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.3847/1538-3881/acdac7$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Cañas, Caleb I</creatorcontrib><creatorcontrib>Kanodia, Shubham</creatorcontrib><creatorcontrib>Libby-Roberts, Jessica</creatorcontrib><creatorcontrib>Lin, Andrea S J</creatorcontrib><creatorcontrib>Schutte, Maria</creatorcontrib><creatorcontrib>Powers, Luke</creatorcontrib><creatorcontrib>Jones, Sinclaire</creatorcontrib><creatorcontrib>Monson, Andrew</creatorcontrib><creatorcontrib>Wang, Songhu</creatorcontrib><creatorcontrib>Stefánsson, Guðmundur</creatorcontrib><creatorcontrib>Cochran, William D</creatorcontrib><creatorcontrib>Robertson, Paul</creatorcontrib><creatorcontrib>Mahadevan, Suvrath</creatorcontrib><creatorcontrib>Kowalski, Adam F</creatorcontrib><creatorcontrib>Wisniewski, John</creatorcontrib><creatorcontrib>Parker, Brock A</creatorcontrib><creatorcontrib>Larsen, Alexander</creatorcontrib><creatorcontrib>Chapman, Franklin A L</creatorcontrib><creatorcontrib>Kobulnicky, Henry A</creatorcontrib><creatorcontrib>Gupta, Arvind F</creatorcontrib><creatorcontrib>Everett, Mark E</creatorcontrib><creatorcontrib>Penprase, Bryan Edward</creatorcontrib><creatorcontrib>Zeimann, Gregory</creatorcontrib><creatorcontrib>Beard, Corey</creatorcontrib><creatorcontrib>Bender, Chad F</creatorcontrib><creatorcontrib>Colón, Knicole D</creatorcontrib><creatorcontrib>Diddams, Scott A</creatorcontrib><creatorcontrib>Connor, Fredrick</creatorcontrib><creatorcontrib>Halverson, Samuel</creatorcontrib><creatorcontrib>Ninan, Joe P</creatorcontrib><creatorcontrib>Ramsey, Lawrence W</creatorcontrib><creatorcontrib>Roy, Arpita</creatorcontrib><creatorcontrib>Schwab, Christian</creatorcontrib><title>TOI-3984 A b and TOI-5293 A b: two temperate gas giants transiting mid-M dwarfs in wide binary systems</title><title>arXiv.org</title><description>We confirm the planetary nature of two gas giants discovered by TESS to transit M dwarfs with stellar companions at wide separations. TOI-3984 A (\(J=11.93\)) is an M4 dwarf hosting a short-period (\(4.353326 \pm 0.000005\) days) gas giant (\(M_p=0.14\pm0.03~\mathrm{M_{J}}\) and \(R_p=0.71\pm0.02~\mathrm{R_{J}}\)) with a wide separation white dwarf companion. TOI-5293 A (\(J=12.47\)) is an M3 dwarf hosting a short-period (\(2.930289 \pm 0.000004\) days) gas giant (\(M_p=0.54\pm0.07~\mathrm{M_{J}}\) and \(R_p=1.06\pm0.04~\mathrm{R_{J}}\)) with a wide separation M dwarf companion. We characterize both systems using a combination of ground-based and space-based photometry, speckle imaging, and high-precision radial velocities from the Habitable-zone Planet Finder and NEID spectrographs. TOI-3984 A b (\(T_{eq}=563\pm15\) K and \(\mathrm{TSM}=138_{-27}^{+29}\)) and TOI-5293 A b (\(T_{eq}=675_{-30}^{+42}\) K and \(\mathrm{TSM}=92\pm14\)) are two of the coolest gas giants among the population of hot Jupiter-sized gas planets orbiting M dwarfs and are favorable targets for atmospheric characterization of temperate gas giants and three-dimensional obliquity measurements to probe system architecture and migration scenarios.</description><subject>Binary stars</subject><subject>Circumstellar habitable zone</subject><subject>Computer architecture</subject><subject>Extrasolar planets</subject><subject>Gas giant planets</subject><subject>Jupiter</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><subject>Red dwarf stars</subject><subject>Separation</subject><subject>Spectrographs</subject><subject>White dwarf stars</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotkMtqQjEURUOhULF-QEc90PG1uXmnM5E-BIsT55cjSSRSo01irX_fq3Z0YLP2YbMIeWjpWBgp6TPm3_gzZpyyMdW6FTdkwDhvGyMYuyOjUjaUUqY0k5IPSFguZg23RsAEVoDJwTmQzPJz8AL1uIPqt3ufsXpYY4F1xFQL1IypxBrTGrbRNZ_gjphDgZjgGJ2HVUyYT1BOpa-Xe3Ib8Kv40f8dkuXb63L60cwX77PpZN6glaIxJliULSojlVRWK8uVEzKg88xooXxPmRbRKBcUDd7jyiLzWolWaYOaD8nj9e1FQrfPcduP6M4yuouMnni6Evu8-z74UrvN7pBTv6ljuieUFVTzP-bdXtU</recordid><startdate>20230627</startdate><enddate>20230627</enddate><creator>Cañas, Caleb I</creator><creator>Kanodia, Shubham</creator><creator>Libby-Roberts, Jessica</creator><creator>Lin, Andrea S J</creator><creator>Schutte, Maria</creator><creator>Powers, Luke</creator><creator>Jones, Sinclaire</creator><creator>Monson, Andrew</creator><creator>Wang, Songhu</creator><creator>Stefánsson, Guðmundur</creator><creator>Cochran, William D</creator><creator>Robertson, Paul</creator><creator>Mahadevan, Suvrath</creator><creator>Kowalski, Adam F</creator><creator>Wisniewski, John</creator><creator>Parker, Brock A</creator><creator>Larsen, Alexander</creator><creator>Chapman, Franklin A L</creator><creator>Kobulnicky, Henry A</creator><creator>Gupta, Arvind F</creator><creator>Everett, Mark E</creator><creator>Penprase, Bryan Edward</creator><creator>Zeimann, Gregory</creator><creator>Beard, Corey</creator><creator>Bender, Chad F</creator><creator>Colón, Knicole D</creator><creator>Diddams, Scott A</creator><creator>Connor, Fredrick</creator><creator>Halverson, Samuel</creator><creator>Ninan, Joe P</creator><creator>Ramsey, Lawrence W</creator><creator>Roy, Arpita</creator><creator>Schwab, Christian</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20230627</creationdate><title>TOI-3984 A b and TOI-5293 A b: two temperate gas giants transiting mid-M dwarfs in wide binary systems</title><author>Cañas, Caleb I ; Kanodia, Shubham ; Libby-Roberts, Jessica ; Lin, Andrea S J ; Schutte, Maria ; Powers, Luke ; Jones, Sinclaire ; Monson, Andrew ; Wang, Songhu ; Stefánsson, Guðmundur ; Cochran, William D ; Robertson, Paul ; Mahadevan, Suvrath ; Kowalski, Adam F ; Wisniewski, John ; Parker, Brock A ; Larsen, Alexander ; Chapman, Franklin A L ; Kobulnicky, Henry A ; Gupta, Arvind F ; Everett, Mark E ; Penprase, Bryan Edward ; Zeimann, Gregory ; Beard, Corey ; Bender, Chad F ; Colón, Knicole D ; Diddams, Scott A ; Connor, Fredrick ; Halverson, Samuel ; Ninan, Joe P ; Ramsey, Lawrence W ; Roy, Arpita ; Schwab, Christian</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a954-88f9a51a685656976936d45fade28746ea9581aa86df60feeab9a2e7641678a73</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Binary stars</topic><topic>Circumstellar habitable zone</topic><topic>Computer architecture</topic><topic>Extrasolar planets</topic><topic>Gas giant planets</topic><topic>Jupiter</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><topic>Red dwarf stars</topic><topic>Separation</topic><topic>Spectrographs</topic><topic>White dwarf stars</topic><toplevel>online_resources</toplevel><creatorcontrib>Cañas, Caleb I</creatorcontrib><creatorcontrib>Kanodia, Shubham</creatorcontrib><creatorcontrib>Libby-Roberts, Jessica</creatorcontrib><creatorcontrib>Lin, Andrea S J</creatorcontrib><creatorcontrib>Schutte, Maria</creatorcontrib><creatorcontrib>Powers, Luke</creatorcontrib><creatorcontrib>Jones, Sinclaire</creatorcontrib><creatorcontrib>Monson, Andrew</creatorcontrib><creatorcontrib>Wang, Songhu</creatorcontrib><creatorcontrib>Stefánsson, Guðmundur</creatorcontrib><creatorcontrib>Cochran, William D</creatorcontrib><creatorcontrib>Robertson, Paul</creatorcontrib><creatorcontrib>Mahadevan, Suvrath</creatorcontrib><creatorcontrib>Kowalski, Adam F</creatorcontrib><creatorcontrib>Wisniewski, John</creatorcontrib><creatorcontrib>Parker, Brock A</creatorcontrib><creatorcontrib>Larsen, Alexander</creatorcontrib><creatorcontrib>Chapman, Franklin A L</creatorcontrib><creatorcontrib>Kobulnicky, Henry A</creatorcontrib><creatorcontrib>Gupta, Arvind F</creatorcontrib><creatorcontrib>Everett, Mark E</creatorcontrib><creatorcontrib>Penprase, Bryan Edward</creatorcontrib><creatorcontrib>Zeimann, Gregory</creatorcontrib><creatorcontrib>Beard, Corey</creatorcontrib><creatorcontrib>Bender, Chad F</creatorcontrib><creatorcontrib>Colón, Knicole D</creatorcontrib><creatorcontrib>Diddams, Scott A</creatorcontrib><creatorcontrib>Connor, Fredrick</creatorcontrib><creatorcontrib>Halverson, Samuel</creatorcontrib><creatorcontrib>Ninan, Joe P</creatorcontrib><creatorcontrib>Ramsey, Lawrence W</creatorcontrib><creatorcontrib>Roy, Arpita</creatorcontrib><creatorcontrib>Schwab, Christian</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Cañas, Caleb I</au><au>Kanodia, Shubham</au><au>Libby-Roberts, Jessica</au><au>Lin, Andrea S J</au><au>Schutte, Maria</au><au>Powers, Luke</au><au>Jones, Sinclaire</au><au>Monson, Andrew</au><au>Wang, Songhu</au><au>Stefánsson, Guðmundur</au><au>Cochran, William D</au><au>Robertson, Paul</au><au>Mahadevan, Suvrath</au><au>Kowalski, Adam F</au><au>Wisniewski, John</au><au>Parker, Brock A</au><au>Larsen, Alexander</au><au>Chapman, Franklin A L</au><au>Kobulnicky, Henry A</au><au>Gupta, Arvind F</au><au>Everett, Mark E</au><au>Penprase, Bryan Edward</au><au>Zeimann, Gregory</au><au>Beard, Corey</au><au>Bender, Chad F</au><au>Colón, Knicole D</au><au>Diddams, Scott A</au><au>Connor, Fredrick</au><au>Halverson, Samuel</au><au>Ninan, Joe P</au><au>Ramsey, Lawrence W</au><au>Roy, Arpita</au><au>Schwab, Christian</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>TOI-3984 A b and TOI-5293 A b: two temperate gas giants transiting mid-M dwarfs in wide binary systems</atitle><jtitle>arXiv.org</jtitle><date>2023-06-27</date><risdate>2023</risdate><eissn>2331-8422</eissn><abstract>We confirm the planetary nature of two gas giants discovered by TESS to transit M dwarfs with stellar companions at wide separations. TOI-3984 A (\(J=11.93\)) is an M4 dwarf hosting a short-period (\(4.353326 \pm 0.000005\) days) gas giant (\(M_p=0.14\pm0.03~\mathrm{M_{J}}\) and \(R_p=0.71\pm0.02~\mathrm{R_{J}}\)) with a wide separation white dwarf companion. TOI-5293 A (\(J=12.47\)) is an M3 dwarf hosting a short-period (\(2.930289 \pm 0.000004\) days) gas giant (\(M_p=0.54\pm0.07~\mathrm{M_{J}}\) and \(R_p=1.06\pm0.04~\mathrm{R_{J}}\)) with a wide separation M dwarf companion. We characterize both systems using a combination of ground-based and space-based photometry, speckle imaging, and high-precision radial velocities from the Habitable-zone Planet Finder and NEID spectrographs. TOI-3984 A b (\(T_{eq}=563\pm15\) K and \(\mathrm{TSM}=138_{-27}^{+29}\)) and TOI-5293 A b (\(T_{eq}=675_{-30}^{+42}\) K and \(\mathrm{TSM}=92\pm14\)) are two of the coolest gas giants among the population of hot Jupiter-sized gas planets orbiting M dwarfs and are favorable targets for atmospheric characterization of temperate gas giants and three-dimensional obliquity measurements to probe system architecture and migration scenarios.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2302.07714</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Binary stars Circumstellar habitable zone Computer architecture Extrasolar planets Gas giant planets Jupiter Physics - Earth and Planetary Astrophysics Physics - Solar and Stellar Astrophysics Red dwarf stars Separation Spectrographs White dwarf stars |
| title | TOI-3984 A b and TOI-5293 A b: two temperate gas giants transiting mid-M dwarfs in wide binary systems |
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