Buchumschlag

HARPS-N, TESS, and CHEOPS discover a transiting sub-Neptune and two outer companions around the bright solar analogue HD 85426

Fuente: arXiv

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Bibliographische Detailangaben
Hauptverfasser:	Lienhard, F., Mortier, A., Cameron, A. Collier, Cretignier, M., Borsato, L., John, A. Anna, Egger, J. A., Stalport, M., Wilson, T. G., Deline, A., Fortier, A., Latham, D. W., Malavolta, L., Maxted, P. F. L., Sousa, S. G., Grimm, S. L., Buchhave, L., Alibert, Y., Lakeland, B. S., Dumusque, X., Cabrera, J., Naponiello, L., Correia, A. C. M., Rescigno, F., Fossati, L., Sozzetti, A., Alonso, R., Bárczy, T., Barrado, D., Barros, S. C. C., Baumjohann, W., Benz, W., Billot, N., Brandeker, A., Broeg, C., Collins, K., Csizmadia, Sz., Cubillos, P. E., Davies, M. B., Deleuil, M., Demangeon, O. D. S., Demory, B. -O., Derekas, A., Edwards, B., Ehrenreich, D., Erikson, A., Fridlund, M., Gandolfi, D., Gazeas, K., Gillon, M., Güdel, M., Günther, M. N., Haywood, R., Heitzmann, A., Helling, Ch., Isaak, K. G., Jenkins, J. M., Kiss, L. L., Korth, J., Lam, K. W. F., Laskar, J., Etangs, A. Lecavelier des, Leleu, A., Lendl, M., Magrin, D., Fiorenzano, A. F. Martínez, Merín, B., Mordasini, C., Nascimbeni, V., Olofsson, G., Osborn, H. P., Ottensamer, R., Pagano, I., Palethorpe, L., Pallé, E., Peter, G., Piazza, D., Piotto, G., Pollacco, D., Queloz, D., Ragazzoni, R., Rando, N., Rauer, H., Ribas, I., Rice, K., Santos, N. C., Scandariato, G., Ségransan, D., Simon, A. E., Smith, A. M. S., Sulis, S., Szabó, Gy. M., Udry, S., Ulmer-Moll, S., Van Grootel, V., Venturini, J., Villaver, E., Walton, N. A., Zingales, T.
Format:	Preprint
Veröffentlicht:	2025
Schlagworte:	Earth and Planetary Astrophysics
Online-Zugang:	Acceder al recurso
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author	Lienhard, F. Mortier, A. Cameron, A. Collier Cretignier, M. Borsato, L. John, A. Anna Egger, J. A. Stalport, M. Wilson, T. G. Deline, A. Fortier, A. Latham, D. W. Malavolta, L. Maxted, P. F. L. Sousa, S. G. Grimm, S. L. Buchhave, L. Alibert, Y. Lakeland, B. S. Dumusque, X. Cabrera, J. Naponiello, L. Correia, A. C. M. Rescigno, F. Fossati, L. Sozzetti, A. Alonso, R. Bárczy, T. Barrado, D. Barros, S. C. C. Baumjohann, W. Benz, W. Billot, N. Brandeker, A. Broeg, C. Collins, K. Csizmadia, Sz. Cubillos, P. E. Davies, M. B. Deleuil, M. Demangeon, O. D. S. Demory, B. -O. Derekas, A. Edwards, B. Ehrenreich, D. Erikson, A. Fridlund, M. Gandolfi, D. Gazeas, K. Gillon, M. Güdel, M. Günther, M. N. Haywood, R. Heitzmann, A. Helling, Ch. Isaak, K. G. Jenkins, J. M. Kiss, L. L. Korth, J. Lam, K. W. F. Laskar, J. Etangs, A. Lecavelier des Leleu, A. Lendl, M. Magrin, D. Fiorenzano, A. F. Martínez Merín, B. Mordasini, C. Nascimbeni, V. Olofsson, G. Osborn, H. P. Ottensamer, R. Pagano, I. Palethorpe, L. Pallé, E. Peter, G. Piazza, D. Piotto, G. Pollacco, D. Queloz, D. Ragazzoni, R. Rando, N. Rauer, H. Ribas, I. Rice, K. Santos, N. C. Scandariato, G. Ségransan, D. Simon, A. E. Smith, A. M. S. Sulis, S. Szabó, Gy. M. Udry, S. Ulmer-Moll, S. Van Grootel, V. Venturini, J. Villaver, E. Walton, N. A. Zingales, T.
author_facet	Lienhard, F. Mortier, A. Cameron, A. Collier Cretignier, M. Borsato, L. John, A. Anna Egger, J. A. Stalport, M. Wilson, T. G. Deline, A. Fortier, A. Latham, D. W. Malavolta, L. Maxted, P. F. L. Sousa, S. G. Grimm, S. L. Buchhave, L. Alibert, Y. Lakeland, B. S. Dumusque, X. Cabrera, J. Naponiello, L. Correia, A. C. M. Rescigno, F. Fossati, L. Sozzetti, A. Alonso, R. Bárczy, T. Barrado, D. Barros, S. C. C. Baumjohann, W. Benz, W. Billot, N. Brandeker, A. Broeg, C. Collins, K. Csizmadia, Sz. Cubillos, P. E. Davies, M. B. Deleuil, M. Demangeon, O. D. S. Demory, B. -O. Derekas, A. Edwards, B. Ehrenreich, D. Erikson, A. Fridlund, M. Gandolfi, D. Gazeas, K. Gillon, M. Güdel, M. Günther, M. N. Haywood, R. Heitzmann, A. Helling, Ch. Isaak, K. G. Jenkins, J. M. Kiss, L. L. Korth, J. Lam, K. W. F. Laskar, J. Etangs, A. Lecavelier des Leleu, A. Lendl, M. Magrin, D. Fiorenzano, A. F. Martínez Merín, B. Mordasini, C. Nascimbeni, V. Olofsson, G. Osborn, H. P. Ottensamer, R. Pagano, I. Palethorpe, L. Pallé, E. Peter, G. Piazza, D. Piotto, G. Pollacco, D. Queloz, D. Ragazzoni, R. Rando, N. Rauer, H. Ribas, I. Rice, K. Santos, N. C. Scandariato, G. Ségransan, D. Simon, A. E. Smith, A. M. S. Sulis, S. Szabó, Gy. M. Udry, S. Ulmer-Moll, S. Van Grootel, V. Venturini, J. Villaver, E. Walton, N. A. Zingales, T.
contents	We provide a detailed characterisation of the planetary system orbiting HD 85426 (TOI-1774). This bright G-type star ($M_{\ast}$: 0.99 $\text{M}_{\odot}$; $R_{\ast}$: 1.13 $\text{R}_{\odot}$; age: 7.4 Gyr; V mag: 8.25) hosts a transiting sub-Neptune, HD 85426 b, with an orbital period of 16.71 days and a blackbody equilibrium temperature of $824^{+11}_{-11}$ K. By jointly analysing HARPS-N RVs, TESS, and CHEOPS photometric data and using two different stellar activity mitigation techniques, we constrain planet b's mass to $6.0^{+1.5}_{-1.6}$ $\text{M}_{\oplus}$ and $8.5^{+1.3}_{-1.4} $ $\text{M}_{\oplus}$, depending on the mitigation technique. We investigate the dependence of these results on the priors, data selection, and inclusion of other Keplerians in the modelling. Using this approach, we identify the presence of two non-transiting planetary companions with minimum masses near 10 $\text{M}_{\oplus}$ and orbital periods of 35.7 and 89 days. Additionally, we reject the initial hypothesis that the 35.7-day periodic signal was due to stellar activity. We also determine HD 85426 b's radius to be $2.78^{+0.05}_{-0.04}$ $\text{R}_{\oplus}$ and compute a transmission spectroscopy metric in the range of 82 to 115, making this planet a highly valuable target for atmospheric characterisation.
format	Preprint
id	arxiv_https___arxiv_org_abs_2511_08473
institution	arXiv
publishDate	2025
record_format	arxiv
spellingShingle	HARPS-N, TESS, and CHEOPS discover a transiting sub-Neptune and two outer companions around the bright solar analogue HD 85426 Lienhard, F. Mortier, A. Cameron, A. Collier Cretignier, M. Borsato, L. John, A. Anna Egger, J. A. Stalport, M. Wilson, T. G. Deline, A. Fortier, A. Latham, D. W. Malavolta, L. Maxted, P. F. L. Sousa, S. G. Grimm, S. L. Buchhave, L. Alibert, Y. Lakeland, B. S. Dumusque, X. Cabrera, J. Naponiello, L. Correia, A. C. M. Rescigno, F. Fossati, L. Sozzetti, A. Alonso, R. Bárczy, T. Barrado, D. Barros, S. C. C. Baumjohann, W. Benz, W. Billot, N. Brandeker, A. Broeg, C. Collins, K. Csizmadia, Sz. Cubillos, P. E. Davies, M. B. Deleuil, M. Demangeon, O. D. S. Demory, B. -O. Derekas, A. Edwards, B. Ehrenreich, D. Erikson, A. Fridlund, M. Gandolfi, D. Gazeas, K. Gillon, M. Güdel, M. Günther, M. N. Haywood, R. Heitzmann, A. Helling, Ch. Isaak, K. G. Jenkins, J. M. Kiss, L. L. Korth, J. Lam, K. W. F. Laskar, J. Etangs, A. Lecavelier des Leleu, A. Lendl, M. Magrin, D. Fiorenzano, A. F. Martínez Merín, B. Mordasini, C. Nascimbeni, V. Olofsson, G. Osborn, H. P. Ottensamer, R. Pagano, I. Palethorpe, L. Pallé, E. Peter, G. Piazza, D. Piotto, G. Pollacco, D. Queloz, D. Ragazzoni, R. Rando, N. Rauer, H. Ribas, I. Rice, K. Santos, N. C. Scandariato, G. Ségransan, D. Simon, A. E. Smith, A. M. S. Sulis, S. Szabó, Gy. M. Udry, S. Ulmer-Moll, S. Van Grootel, V. Venturini, J. Villaver, E. Walton, N. A. Zingales, T. Earth and Planetary Astrophysics We provide a detailed characterisation of the planetary system orbiting HD 85426 (TOI-1774). This bright G-type star ($M_{\ast}$: 0.99 $\text{M}_{\odot}$; $R_{\ast}$: 1.13 $\text{R}_{\odot}$; age: 7.4 Gyr; V mag: 8.25) hosts a transiting sub-Neptune, HD 85426 b, with an orbital period of 16.71 days and a blackbody equilibrium temperature of $824^{+11}_{-11}$ K. By jointly analysing HARPS-N RVs, TESS, and CHEOPS photometric data and using two different stellar activity mitigation techniques, we constrain planet b's mass to $6.0^{+1.5}_{-1.6}$ $\text{M}_{\oplus}$ and $8.5^{+1.3}_{-1.4} $ $\text{M}_{\oplus}$, depending on the mitigation technique. We investigate the dependence of these results on the priors, data selection, and inclusion of other Keplerians in the modelling. Using this approach, we identify the presence of two non-transiting planetary companions with minimum masses near 10 $\text{M}_{\oplus}$ and orbital periods of 35.7 and 89 days. Additionally, we reject the initial hypothesis that the 35.7-day periodic signal was due to stellar activity. We also determine HD 85426 b's radius to be $2.78^{+0.05}_{-0.04}$ $\text{R}_{\oplus}$ and compute a transmission spectroscopy metric in the range of 82 to 115, making this planet a highly valuable target for atmospheric characterisation.
title	HARPS-N, TESS, and CHEOPS discover a transiting sub-Neptune and two outer companions around the bright solar analogue HD 85426
topic	Earth and Planetary Astrophysics
url	https://arxiv.org/abs/2511.08473