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Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076

Authors :
Osborn, Hugh P.
Bonfanti, Andrea
Gandolfi, Davide
Hedges, Christina
Leleu, Adrien
Fortier, Andrea
Futyan, David
Gutermann, Pascal
Maxted, Pierre F. L.
Borsato, Luca
Collins, Karen A.
da Silva, J. Gomes
Chew, Yilen Gómez Maqueo
Hooton, Matthew J.
Lendl, Monika
Parviainen, Hannu
Salmon, Sébastien
Schanche, Nicole
Serrano, Luisa M.
Sousa, Sergio G.
Tuson, Amy
Ulmer-Moll, Solène
Van Grootel, Valerie
Wells, R. D.
Wilson, Thomas G.
Alibert, Yann
Alonso, Roi
Anglada, Guillem
Asquier, Joel
Navascues, David Barrado y
Baumjohann, Wolfgang
Beck, Thomas
Benz, Willy
Biondi, Federico
Bonfils, Xavier
Bouchy, Francois
Brandeker, Alexis
Broeg, Christopher
Bárczy, Tamas
Barros, S. C. C.
Cabrera, Juan
Charnoz, Sébastien
Cameron, Andrew Collier
Csizmadia, Szilard
Davies, Melvyn B.
Deleuil, Magali
Delrez, Laetitia
Demory, Brice-Olivier
Ehrenreich, David
Erikson, Anders
Fossati, Luca
Fridlund, Malcolm
Gillon, Michaël
Gómez-Muñoz, M. A.
Güdel, Manuel
Heng, Kevin
Hoyer, Sergio
Isaak, Kate G.
Kiss, Laszlo
Laskar, Jacques
Etangs, Alain Lecavelier des
Lovis, Christophe
Magrin, Demetrio
Malavolta, Luca
McCormac, James
Nascimbeni, Valerio
Olofsson, Göran
Ottensamer, Roland
Pagano, Isabella
Pallé, Enric
Peter, Gisbert
Piazza, Daniele
Piotto, Giampaolo
Pollacco, Don
Queloz, Didier
Ragazzoni, Roberto
Rando, Nicola
Rauer, Heike
Reimers, Christian
Ribas, Ignasi
Demangeon, Olivier D. S.
Smith, Alexis M. S.
Sabin, L.
Santos, Nuno
Scandariato, Gaetano
Schroffenegger, U.
Schwarz, Rick P.
Shporer, Avi
Simon, Attila E.
Steller, Manfred
Szabó, Gyula M.
Ségransan, Damien
Thomas, Nicolas
Udry, Stéphane
Walter, Ingo
Walton, Nicholas
Osborn, Hugh P.
Bonfanti, Andrea
Gandolfi, Davide
Hedges, Christina
Leleu, Adrien
Fortier, Andrea
Futyan, David
Gutermann, Pascal
Maxted, Pierre F. L.
Borsato, Luca
Collins, Karen A.
da Silva, J. Gomes
Chew, Yilen Gómez Maqueo
Hooton, Matthew J.
Lendl, Monika
Parviainen, Hannu
Salmon, Sébastien
Schanche, Nicole
Serrano, Luisa M.
Sousa, Sergio G.
Tuson, Amy
Ulmer-Moll, Solène
Van Grootel, Valerie
Wells, R. D.
Wilson, Thomas G.
Alibert, Yann
Alonso, Roi
Anglada, Guillem
Asquier, Joel
Navascues, David Barrado y
Baumjohann, Wolfgang
Beck, Thomas
Benz, Willy
Biondi, Federico
Bonfils, Xavier
Bouchy, Francois
Brandeker, Alexis
Broeg, Christopher
Bárczy, Tamas
Barros, S. C. C.
Cabrera, Juan
Charnoz, Sébastien
Cameron, Andrew Collier
Csizmadia, Szilard
Davies, Melvyn B.
Deleuil, Magali
Delrez, Laetitia
Demory, Brice-Olivier
Ehrenreich, David
Erikson, Anders
Fossati, Luca
Fridlund, Malcolm
Gillon, Michaël
Gómez-Muñoz, M. A.
Güdel, Manuel
Heng, Kevin
Hoyer, Sergio
Isaak, Kate G.
Kiss, Laszlo
Laskar, Jacques
Etangs, Alain Lecavelier des
Lovis, Christophe
Magrin, Demetrio
Malavolta, Luca
McCormac, James
Nascimbeni, Valerio
Olofsson, Göran
Ottensamer, Roland
Pagano, Isabella
Pallé, Enric
Peter, Gisbert
Piazza, Daniele
Piotto, Giampaolo
Pollacco, Don
Queloz, Didier
Ragazzoni, Roberto
Rando, Nicola
Rauer, Heike
Reimers, Christian
Ribas, Ignasi
Demangeon, Olivier D. S.
Smith, Alexis M. S.
Sabin, L.
Santos, Nuno
Scandariato, Gaetano
Schroffenegger, U.
Schwarz, Rick P.
Shporer, Avi
Simon, Attila E.
Steller, Manfred
Szabó, Gyula M.
Ségransan, Damien
Thomas, Nicolas
Udry, Stéphane
Walter, Ingo
Walton, Nicholas
Publication Year :
2022

Abstract

Context: TOI-2076 is a transiting three-planet system of sub-Neptunes orbiting a bright (G = 8.9 mag), young ($340\pm80$ Myr) K-type star. Although a validated planetary system, the orbits of the two outer planets were unconstrained as only two non-consecutive transits were seen in TESS photometry. This left 11 and 7 possible period aliases for each. Aims: To reveal the true orbits of these two long-period planets, precise photometry targeted on the highest-probability period aliases is required. Long-term monitoring of transits in multi-planet systems can also help constrain planetary masses through TTV measurements. Methods: We used the MonoTools package to determine which aliases to follow, and then performed space-based and ground-based photometric follow-up of TOI-2076 c and d with CHEOPS, SAINT-EX, and LCO telescopes. Results: CHEOPS observations revealed a clear detection for TOI-2076 c at $P=21.01538^{+0.00084}_{-0.00074}$ d, and allowed us to rule out three of the most likely period aliases for TOI-2076 d. Ground-based photometry further enabled us to rule out remaining aliases and confirm the $P=35.12537\pm0.00067$ d alias. These observations also improved the radius precision of all three sub-Neptunes to $2.518\pm0.036$, $3.497\pm0.043$, and $3.232\pm0.063$ $R_\oplus$. Our observations also revealed a clear anti-correlated TTV signal between planets b and c likely caused by their proximity to the 2:1 resonance, while planets c and d appear close to a 5:3 period commensurability, although model degeneracy meant we were unable to retrieve robust TTV masses. Their inflated radii, likely due to extended H-He atmospheres, combined with low insolation makes all three planets excellent candidates for future comparative transmission spectroscopy with JWST.<br />Comment: 18 pages, 7 figure, 8 tables. Accepted for publication in Astronomy & Astrophysics. Photometry available on CDS/Vizier. Python package presented for modelling duotransiting planet candidates available at https://github.com/hposborn/MonoTools. Modelling & figure-creation code available at https://github.com/hposborn/TOI2076

Details

Database :
OAIster
Publication Type :
Electronic Resource
Accession number :
edsoai.on1312096928
Document Type :
Electronic Resource
Full Text :
https://doi.org/10.1051.0004-6361.202243065