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Characterization of seven transiting systems including four warm Jupiters from SOPHIE and TESS

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Heidari, N., H'ebrard, G., Martioli, E., Eastman, J. D., Jackson, J. M., Delfosse, X., Jord'an, A., Correia, A. C. M., Sousa, S., Dragomir, D., Forveille, T., Boisse, I., Giacalone, S. A., D'iaz, R. F., Brahm, R., Almasian, D., Almenara, J. M., Bieryla, A., Barkaoui, K., Baker, D., Barros, S. C. C ., Bonfils, X., Carmona, A., Collins, K. A., Cort'es-Zuleta, P., Deleuil, M., Demangeon, O. D. S., Edwards, B., Eberhardt, J., Espinoza, N., Eisner, N., Feliz, D. L., Frommer, A. C., Fukui, A., Grau, F., Gupta, A. F., Hara, N., Hobson, M. J., Henning, T., Howell, S. B., Jenkins, J. M., Kiefer, F., LaCourse, D. M., Laskar, J., Law, N., Mann, A. W., Murgas, F., Moutou, C., Narita, N., Palle, E., Relles, H. M., Stassun, K. G., Bell, J. Serrano, Schwarz, R. P., Srdoc, G., Strøm, P. A., Safonov, B., Sarkis, P., Schlecker, M., Pinto, M. Tala, Pepper, J., Rojas, F. I., Twicken, J. D., Trifonov, T., Villanueva Jr, S., Watkins, C. N., Winn, J. N., Ziegler, C.
Formato:	Preprint
Publicado:	2024
Materias:	Earth and Planetary Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

_version_	1866909487593422848
author	Heidari, N. H'ebrard, G. Martioli, E. Eastman, J. D. Jackson, J. M. Delfosse, X. Jord'an, A. Correia, A. C. M. Sousa, S. Dragomir, D. Forveille, T. Boisse, I. Giacalone, S. A. D'iaz, R. F. Brahm, R. Almasian, D. Almenara, J. M. Bieryla, A. Barkaoui, K. Baker, D. Barros, S. C. C . Bonfils, X. Carmona, A. Collins, K. A. Cort'es-Zuleta, P. Deleuil, M. Demangeon, O. D. S. Edwards, B. Eberhardt, J. Espinoza, N. Eisner, N. Feliz, D. L. Frommer, A. C. Fukui, A. Grau, F. Gupta, A. F. Hara, N. Hobson, M. J. Henning, T. Howell, S. B. Jenkins, J. M. Kiefer, F. LaCourse, D. M. Laskar, J. Law, N. Mann, A. W. Murgas, F. Moutou, C. Narita, N. Palle, E. Relles, H. M. Stassun, K. G. Bell, J. Serrano Schwarz, R. P. Srdoc, G. Strøm, P. A. Safonov, B. Sarkis, P. Schlecker, M. Pinto, M. Tala Pepper, J. Rojas, F. I. Twicken, J. D. Trifonov, T. Villanueva Jr, S. Watkins, C. N. Winn, J. N. Ziegler, C.
author_facet	Heidari, N. H'ebrard, G. Martioli, E. Eastman, J. D. Jackson, J. M. Delfosse, X. Jord'an, A. Correia, A. C. M. Sousa, S. Dragomir, D. Forveille, T. Boisse, I. Giacalone, S. A. D'iaz, R. F. Brahm, R. Almasian, D. Almenara, J. M. Bieryla, A. Barkaoui, K. Baker, D. Barros, S. C. C . Bonfils, X. Carmona, A. Collins, K. A. Cort'es-Zuleta, P. Deleuil, M. Demangeon, O. D. S. Edwards, B. Eberhardt, J. Espinoza, N. Eisner, N. Feliz, D. L. Frommer, A. C. Fukui, A. Grau, F. Gupta, A. F. Hara, N. Hobson, M. J. Henning, T. Howell, S. B. Jenkins, J. M. Kiefer, F. LaCourse, D. M. Laskar, J. Law, N. Mann, A. W. Murgas, F. Moutou, C. Narita, N. Palle, E. Relles, H. M. Stassun, K. G. Bell, J. Serrano Schwarz, R. P. Srdoc, G. Strøm, P. A. Safonov, B. Sarkis, P. Schlecker, M. Pinto, M. Tala Pepper, J. Rojas, F. I. Twicken, J. D. Trifonov, T. Villanueva Jr, S. Watkins, C. N. Winn, J. N. Ziegler, C.
contents	We present the study of seven systems, three of which TOI-2295, TOI-2537, and TOI-5110 are newly discovered planetary systems. Through the analysis of TESS photometry, SOPHIE radial velocities, and high-spatial resolution imaging, we found that TOI-2295b, TOI-2537b, and TOI-5110b are transiting warm Jupiters with orbital periods ranging from 30 to 94 d, masses between 0.9 and 2.9 MJ, and radii ranging from 1.0 to 1.5 RJ. Both TOI-2295 and TOI-2537 each harbor at least one additional, outer planet. Their outer planets TOI-2295c and TOI-2537c are characterized by orbital periods of 966.5 +/- 4.3 and 1920^{+230}_{-140} d, respectively, and minimum masses of 5.61^{+0.23}_{-0.24} and 7.2 +/- 0.5 MJ, respectively. We also investigated and characterized the two recently reported warm Jupiters TOI-1836b and TOI-5076b, which we independently detected in SOPHIE RVs. Additionally, we study the planetary candidates TOI-4081.01 and TOI-4168.01. For TOI-4081.01, despite our detection in radial velocities, we cannot rule out perturbation by a blended eclipsing binary and thus exercise caution regarding its planetary nature. On the other hand, we identify TOI-4168.01 as a firm false positive. Finally, we highlight interesting characteristics of these new planetary systems. The transits of TOI-2295b are highly grazing, with an impact parameter of 1.056$^{+0.063}_{-0.043}$. TOI-2537b, in turn, is a temperate Jupiter with an effective temperature of 307+/-15 K and can serve as a valuable low-irradiation control for models of hot Jupiter inflation anomalies. We also detected significant transit timing variations (TTVs) for TOI-2537b, which are likely caused by gravitational interactions with the outer planet TOI-2537c. Finally, TOI-5110b stands out due to its orbital eccentricity of 0.75+/- 0.03, one of the highest planetary eccentricities discovered thus far.
format	Preprint
id	arxiv_https___arxiv_org_abs_2412_08527
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Characterization of seven transiting systems including four warm Jupiters from SOPHIE and TESS Heidari, N. H'ebrard, G. Martioli, E. Eastman, J. D. Jackson, J. M. Delfosse, X. Jord'an, A. Correia, A. C. M. Sousa, S. Dragomir, D. Forveille, T. Boisse, I. Giacalone, S. A. D'iaz, R. F. Brahm, R. Almasian, D. Almenara, J. M. Bieryla, A. Barkaoui, K. Baker, D. Barros, S. C. C . Bonfils, X. Carmona, A. Collins, K. A. Cort'es-Zuleta, P. Deleuil, M. Demangeon, O. D. S. Edwards, B. Eberhardt, J. Espinoza, N. Eisner, N. Feliz, D. L. Frommer, A. C. Fukui, A. Grau, F. Gupta, A. F. Hara, N. Hobson, M. J. Henning, T. Howell, S. B. Jenkins, J. M. Kiefer, F. LaCourse, D. M. Laskar, J. Law, N. Mann, A. W. Murgas, F. Moutou, C. Narita, N. Palle, E. Relles, H. M. Stassun, K. G. Bell, J. Serrano Schwarz, R. P. Srdoc, G. Strøm, P. A. Safonov, B. Sarkis, P. Schlecker, M. Pinto, M. Tala Pepper, J. Rojas, F. I. Twicken, J. D. Trifonov, T. Villanueva Jr, S. Watkins, C. N. Winn, J. N. Ziegler, C. Earth and Planetary Astrophysics We present the study of seven systems, three of which TOI-2295, TOI-2537, and TOI-5110 are newly discovered planetary systems. Through the analysis of TESS photometry, SOPHIE radial velocities, and high-spatial resolution imaging, we found that TOI-2295b, TOI-2537b, and TOI-5110b are transiting warm Jupiters with orbital periods ranging from 30 to 94 d, masses between 0.9 and 2.9 MJ, and radii ranging from 1.0 to 1.5 RJ. Both TOI-2295 and TOI-2537 each harbor at least one additional, outer planet. Their outer planets TOI-2295c and TOI-2537c are characterized by orbital periods of 966.5 +/- 4.3 and 1920^{+230}_{-140} d, respectively, and minimum masses of 5.61^{+0.23}_{-0.24} and 7.2 +/- 0.5 MJ, respectively. We also investigated and characterized the two recently reported warm Jupiters TOI-1836b and TOI-5076b, which we independently detected in SOPHIE RVs. Additionally, we study the planetary candidates TOI-4081.01 and TOI-4168.01. For TOI-4081.01, despite our detection in radial velocities, we cannot rule out perturbation by a blended eclipsing binary and thus exercise caution regarding its planetary nature. On the other hand, we identify TOI-4168.01 as a firm false positive. Finally, we highlight interesting characteristics of these new planetary systems. The transits of TOI-2295b are highly grazing, with an impact parameter of 1.056$^{+0.063}_{-0.043}$. TOI-2537b, in turn, is a temperate Jupiter with an effective temperature of 307+/-15 K and can serve as a valuable low-irradiation control for models of hot Jupiter inflation anomalies. We also detected significant transit timing variations (TTVs) for TOI-2537b, which are likely caused by gravitational interactions with the outer planet TOI-2537c. Finally, TOI-5110b stands out due to its orbital eccentricity of 0.75+/- 0.03, one of the highest planetary eccentricities discovered thus far.
title	Characterization of seven transiting systems including four warm Jupiters from SOPHIE and TESS
topic	Earth and Planetary Astrophysics
url	https://arxiv.org/abs/2412.08527