Hidden Gems in <i>TESS</i> : <tt>SHERLOCK</tt> finds two new rocky planets around nearby M dwarfs

Abstract The Hidden Gems project searches the TESS data for additional planets transiting low-mass stars in confirmed systems. Our goal is to identify planet candidates that are below the detection threshold set by the SPOC and QLP pipelines using SHERLOCK , a specialized pipeline for robust detection and vetting of transit signals in TESS data. We present the discovery of two inner rocky planets in the TOI-237 and TOI-4336 A systems, validated with ground-based photometry from the TRAPPIST, SPECULOOS, ExTrA, and LCO facilities. TOI-237 c has a radius of 1.21 ± 0.04R⊕, orbits its mid-M host star every 1.74 days, and is close to a 3:1 mean-motion resonance with TOI-237 b. TOI-4336 A c has a radius of 1.17 ± 0.06R⊕, and orbits with a period of 7.58 days an M3.5 host star which is part of a hierarchical triple system. We performed model comparison to search for non-zero eccentricities, and found that the circular transit models are statistically favored. Dynamical simulations show that both systems are in stable configurations, and the TTVs expected for the TOI-237 system are of the order of seconds. TOI-237 c and TOI-4336 A c join the high-interest population of warm likely super-Earths below the so-called ”radius valley”. In particular, TOI-237 c is a good candidate for phase curve observations with JWST/MIRI thanks to the small radius of the host star and its short period.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2026-04-15
DOI
https://doi.org/10.1093/mnras/stag710
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
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article

Hidden Gems in TESS : <tt>SHERLOCK</tt> finds two new rocky planets around nearby M dwarfs

Benjamin V. Rackham, M. Gillon, Akihiko Fukui, Adam J. Burgasser et al.
Monthly Notices of the Royal Astronomical Society
Stellar, planetary, and galactic studies
article

Hidden Gems in TESS : <tt>SHERLOCK</tt> finds two new rocky planets around nearby M dwarfs

Benjamin V. Rackham, M. Gillon, Akihiko Fukui, Adam J. Burgasser, Khalid Barkaoui, Bárbara Rojas-Ayala, M. G. Scott, E Ducrot, R P Schwarz, M Dévora-Pajares, B-O Demory, M Ghachoui, G Dransfield, N Narita, G Srdoc, Y Gómez Maqueo Chew, Z Way, F J Pozuelos, A H M J Triaud, S Yalçınkaya, M Timmermans, X Bonfils, S B Howell, Y T Davis, E Jehin, K A Collins, J M Almenara, P P Pedersen
article en

Abstract

Abstract The Hidden Gems project searches the TESS data for additional planets transiting low-mass stars in confirmed systems. Our goal is to identify planet candidates that are below the detection threshold set by the SPOC and QLP pipelines using SHERLOCK , a specialized pipeline for robust detection and vetting of transit signals in TESS data. We present the discovery of two inner rocky planets in the TOI-237 and TOI-4336 A systems, validated with ground-based photometry from the TRAPPIST, SPECULOOS, ExTrA, and LCO facilities. TOI-237 c has a radius of 1.21 ± 0.04R⊕, orbits its mid-M host star every 1.74 days, and is close to a 3:1 mean-motion resonance with TOI-237 b. TOI-4336 A c has a radius of 1.17 ± 0.06R⊕, and orbits with a period of 7.58 days an M3.5 host star which is part of a hierarchical triple system. We performed model comparison to search for non-zero eccentricities, and found that the circular transit models are statistically favored. Dynamical simulations show that both systems are in stable configurations, and the TTVs expected for the TOI-237 system are of the order of seconds. TOI-237 c and TOI-4336 A c join the high-interest population of warm likely super-Earths below the so-called ”radius valley”. In particular, TOI-237 c is a good candidate for phase curve observations with JWST/MIRI thanks to the small radius of the host star and its short period.

Monthly Notices of the Royal Astronomical Society
University of Geneva (CH), University of Bern (CH), Cadi Ayyad University (MA), Ames Research Center (US), Centre National de la Recherche Scientifique (FR), Planetary Science Institute (US), Smithsonian Astrophysical Observatory (US), University of Liège (BE), Universidad Autónoma de la Ciudad de México (MX), Délégation Paris 7 (FR), Universidad de Granada (ES), Georgia State University (US), University of Tarapacá (CL), Université Paris Cité (FR), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Université Paris-Saclay (FR), Observatoire de Paris (FR), Northeast Catholic College (US), Pulkovo Observatory (RU), ETH Zurich (CH), University of California San Diego (US), Sorbonne Université (FR), University of Oxford (GB), Astrophysique, Instrumentation et Modélisation (FR), Astrobiology Center (JP), Laboratoire d’études spatiales et d’instrumentation en astrophysique (FR), Center for Astrophysics Harvard & Smithsonian (US), Institute of Applied Physics (MD), CEA Paris-Saclay (FR), Av Engineering (Czechia) (CZ), Instituto de Astrofísica de Canarias (ES), Tokyo Metropolitan Komaba High School (JP), Astronomy and Space (AU), Instituto de Astrofísica de Andalucía (ES), Massachusetts Institute of Technology (US), The University of Tokyo (JP), University of Birmingham (GB), Universidad Nacional Autónoma de México (MX), Université Grenoble Alpes (FR)
Openalex Percentile: Top 14%
Stellar, planetary, and galactic studies
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