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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2501.04383 |
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| _version_ | 1866910777025232896 |
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| author | Ehrhardt, Juliana Thomas, Luis Kellermann, Hanna Freitag, Christine Grupp, Frank Yee, Samuel W. Winn, Joshua N. Hartman, Joel D. Collins, Karen A. Watkins, Cristilyn N. Stassun, Keivan G. Benni, Paul Bieryla, Allyson Carden, Kylee Checinski, Jacek Cheryasov, Dmitry V. Diamond, Brendan Dowling, Nicholas Dressing, Courtney D. Esparza-Borges, Emma Evans, Phil Forés-Toribio, Raquel Fukui, Akihiko Giacalone, Steven Girardin, Eric Goeke, Robert F. Goessl, Claus Hayashi, Yuya Hopp, Ulrich Jenkins, Jon M. Khan, Isa Laloum, Didier Lark, Adam Latham, David W. de Leon, Jerome Marchini, Alessandro Massey, Bob Munoz, Jose A. Murgas, Felipe Narita, Norio Palle, Enric Papini, Riccardo Parviainen, Hannu Pippert, Jan-Niklas Popowicz, Adam Pritchard, Tyler Quinn, Samuel N. Raetz, Manfred Ries, Christoph Riffeser, Arno Savel, Arjun B. Seager, Sara Schmidt, Michael Striegel, Stephanie Srdoc, Gregor Stockdale, Chris Verna, Gaia Watanabe, David Ziegler, Carl Zöller, Raphael |
| author_facet | Ehrhardt, Juliana Thomas, Luis Kellermann, Hanna Freitag, Christine Grupp, Frank Yee, Samuel W. Winn, Joshua N. Hartman, Joel D. Collins, Karen A. Watkins, Cristilyn N. Stassun, Keivan G. Benni, Paul Bieryla, Allyson Carden, Kylee Checinski, Jacek Cheryasov, Dmitry V. Diamond, Brendan Dowling, Nicholas Dressing, Courtney D. Esparza-Borges, Emma Evans, Phil Forés-Toribio, Raquel Fukui, Akihiko Giacalone, Steven Girardin, Eric Goeke, Robert F. Goessl, Claus Hayashi, Yuya Hopp, Ulrich Jenkins, Jon M. Khan, Isa Laloum, Didier Lark, Adam Latham, David W. de Leon, Jerome Marchini, Alessandro Massey, Bob Munoz, Jose A. Murgas, Felipe Narita, Norio Palle, Enric Papini, Riccardo Parviainen, Hannu Pippert, Jan-Niklas Popowicz, Adam Pritchard, Tyler Quinn, Samuel N. Raetz, Manfred Ries, Christoph Riffeser, Arno Savel, Arjun B. Seager, Sara Schmidt, Michael Striegel, Stephanie Srdoc, Gregor Stockdale, Chris Verna, Gaia Watanabe, David Ziegler, Carl Zöller, Raphael |
| contents | We report the confirmation and characterization of four hot Jupiter-type exoplanets initially detected by TESS: TOI-1295 b, TOI-2580 b, TOI-6016 b, and TOI-6130 b. Using observations with the high-resolution echelle spectrograph MaHPS on the 2.1m telescope at Wendelstein Observatory, together with NEID at Kitt Peak National Observatory and TRES at the Fred Lawrence Whipple Observatory, we confirmed the planetary nature of these four planet candidates. We also performed precise mass measurements. All four planets are found to be hot Jupiters with orbital periods between 2.4 and 4.0 days. The sizes of these planets range from 1.29 to 1.64 Jupiter radii, while their masses range from 0.6 to 1.5 Jupiter masses. Additionally, we investigated whether there are signs of other planets in the systems but have found none. Lastly, we compared the radii of our four objects to the results of an empirical study of radius inflation and see that all four demonstrate a good fit with the current models. These four planets belong to the first array of planets confirmed with MaHPS data, supporting the ability of the spectrograph to detect planets around fainter stars as faint as V=12. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2501_04383 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Confirmation of four hot Jupiters detected by TESS using follow-up spectroscopy from MaHPS at Wendelstein together with NEID and TRES Ehrhardt, Juliana Thomas, Luis Kellermann, Hanna Freitag, Christine Grupp, Frank Yee, Samuel W. Winn, Joshua N. Hartman, Joel D. Collins, Karen A. Watkins, Cristilyn N. Stassun, Keivan G. Benni, Paul Bieryla, Allyson Carden, Kylee Checinski, Jacek Cheryasov, Dmitry V. Diamond, Brendan Dowling, Nicholas Dressing, Courtney D. Esparza-Borges, Emma Evans, Phil Forés-Toribio, Raquel Fukui, Akihiko Giacalone, Steven Girardin, Eric Goeke, Robert F. Goessl, Claus Hayashi, Yuya Hopp, Ulrich Jenkins, Jon M. Khan, Isa Laloum, Didier Lark, Adam Latham, David W. de Leon, Jerome Marchini, Alessandro Massey, Bob Munoz, Jose A. Murgas, Felipe Narita, Norio Palle, Enric Papini, Riccardo Parviainen, Hannu Pippert, Jan-Niklas Popowicz, Adam Pritchard, Tyler Quinn, Samuel N. Raetz, Manfred Ries, Christoph Riffeser, Arno Savel, Arjun B. Seager, Sara Schmidt, Michael Striegel, Stephanie Srdoc, Gregor Stockdale, Chris Verna, Gaia Watanabe, David Ziegler, Carl Zöller, Raphael Earth and Planetary Astrophysics We report the confirmation and characterization of four hot Jupiter-type exoplanets initially detected by TESS: TOI-1295 b, TOI-2580 b, TOI-6016 b, and TOI-6130 b. Using observations with the high-resolution echelle spectrograph MaHPS on the 2.1m telescope at Wendelstein Observatory, together with NEID at Kitt Peak National Observatory and TRES at the Fred Lawrence Whipple Observatory, we confirmed the planetary nature of these four planet candidates. We also performed precise mass measurements. All four planets are found to be hot Jupiters with orbital periods between 2.4 and 4.0 days. The sizes of these planets range from 1.29 to 1.64 Jupiter radii, while their masses range from 0.6 to 1.5 Jupiter masses. Additionally, we investigated whether there are signs of other planets in the systems but have found none. Lastly, we compared the radii of our four objects to the results of an empirical study of radius inflation and see that all four demonstrate a good fit with the current models. These four planets belong to the first array of planets confirmed with MaHPS data, supporting the ability of the spectrograph to detect planets around fainter stars as faint as V=12. |
| title | Confirmation of four hot Jupiters detected by TESS using follow-up spectroscopy from MaHPS at Wendelstein together with NEID and TRES |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2501.04383 |