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Mass estimates of the young TOI-451 transiting planets: multidimensional Gaussian Process on stellar spectroscopic and photometric signals

Abstract:
The young TOI-451 planetary system, aged 125 Myr, provides a unique opportunity to test theories of planetary internal structures and atmospheric mass-loss through examination of its three transiting planets. We present an exhaustive photometric and spectroscopic follow-up to determine the orbital and physical properties of the system. We perform multidimensional Gaussian Process regression with the code pyaneti on spectroscopic time-series and NGTS/LCO light curves to disentangle the stellar and planetary signal in ESPRESSO radial velocities. We show how contemporaneous photometry serves as an activity indicator to inform RV modelling within a multidimensional Gaussian Processes framework. We argue that this can be exploited when spectroscopic observations are adversely affected by low signal-to-noise and/or poor sampling. We estimate the Doppler semi-amplitudes of , , and . This translates in 2 mass estimates for TOI-451 b and d of and ; as well as a mass upper limit for TOI-451 c of . The derived planetary properties suggest that planets c and d contain significant hydrogen-rich envelopes. The inferred parameters of TOI-451 b are consistent with either a rocky world that still retains a small hydrogen envelope or a water world. These insights make the TOI-451 system an ideal laboratory for future follow-up studies aimed at measuring atmospheric compositions, detecting atmospheric mass-loss signatures, and further exploring planetary formation and evolution processes.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/stag087

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Physics - Central
Role:
Author
ORCID:
0000-0003-0563-0493
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Role:
Author
ORCID:
0000-0002-1416-2188
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Role:
Author
ORCID:
0000-0002-8675-182X
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Role:
Author
ORCID:
0009-0007-1053-0004


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Funder identifier:
https://ror.org/001aqnf71
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Funder identifier:
https://ror.org/057g20z61
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Funder identifier:
https://ror.org/02ap3w078
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Funder identifier:
https://ror.org/00yjd3n13


Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
546
Issue:
2
Pages:
stag087
Article number:
stag087
Publication date:
2026-01-14
Acceptance date:
2026-01-12
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
Pubs id:
2361347
UUID:
uuid_1800785d-e0d1-47a4-8a89-5e05bca3356e
Local pid:
pubs:2361347
Source identifiers:
3710682
Deposit date:
2026-01-30
ARK identifier:
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