Searching for GEMS: Characterizing Six Giant Planets Around Cool Dwarfs

Abstract Transiting giant exoplanets around M-dwarf stars (GEMS) are rare, owing to the low-mass host stars. However, the all-sky coverage of TESS has enabled the detection of an increasingly large number of them to enable statistical surveys like the Searching for GEMS survey. As part of this endeavor, we describe the observations of six transiting giant planets, which include precise mass measurements for two GEMS (K2-419Ab, TOI-6034b) and statistical validation for four systems, which includes validation and mass upper limits for three of them (TOI-5218b, TOI-5616b, TOI-5634Ab), while the fourth one—TOI-5414b is classified as a “likely planet.” Our observations include radial velocities from the Habitable-zone Planet Finder on the Hobby–Eberly Telescope, and MAROON-X on Gemini-North, along with photometry and high-contrast imaging from multiple ground-based facilities. In addition to TESS photometry, K2-419Ab was also observed and statistically validated as part of the K2 mission in Campaigns 5 and 18, which provide precise orbital and planetary constraints despite the faint host star and long orbital period of ∼20.4 days. With an equilibrium temperature of only 380 K, K2-419Ab is one of the coolest known well-characterized transiting planets. TOI-6034 has a late F-type companion about 40″ away, making it the first GEMS host star to have an earlier main-sequence binary companion. These confirmations add to the existing small sample of confirmed transiting GEMS.

Authors

Publication Details

Journal
The Astronomical Journal
Published
2024-11-04
DOI
https://doi.org/10.3847/1538-3881/ad7796
Citations
11
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
3.65

Funders

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article

Searching for GEMS: Characterizing Six Giant Planets Around Cool Dwarfs

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11 citations
The Astronomical Journal
Stellar, planetary, and galactic studies
3.65
article

Searching for GEMS: Characterizing Six Giant Planets Around Cool Dwarfs

Zoë L. de Beurs, Samuel Halverson, Joe Philip Ninan, R. Luque, Henry A. Kobulnicky, Franklin Chapman, Lia Marta Bernabò, Scott A. Diddams, Caleb I. Cañas, Brock A. Parker, Chad F. Bender, Michael B. Lund, Jessica E. Libby-Roberts, Arvind F. Gupta, Steve B. Howell, Adam F. Kowalski, N. M. Brown, Shubham Kanodia, Arpita Roy, Ritvik Basant, Gabrielle Ross, Madison Brady, Christian Schwab, Te Han, Jacob L. Bean, Andrew Vanderburg, Andrea S. J. Lin, Catherine A. Clark, Guđmundur Stefánsson, Suzanne L. Hawley, Leslie Hebb, N. Morrell, David R. Ciardi, William D. Cochran, Rae Holcomb, Andrew Monson, Alexander Larsen, Andreas Seifahrt, Allyson Bieryla, Michael Rodruck, Varghese Reji, Alexina Birkholz, Ethan G. Cotter, Nishka Patel, Aubrie Thoms
article en
11 citations

Abstract

Abstract Transiting giant exoplanets around M-dwarf stars (GEMS) are rare, owing to the low-mass host stars. However, the all-sky coverage of TESS has enabled the detection of an increasingly large number of them to enable statistical surveys like the Searching for GEMS survey. As part of this endeavor, we describe the observations of six transiting giant planets, which include precise mass measurements for two GEMS (K2-419Ab, TOI-6034b) and statistical validation for four systems, which includes validation and mass upper limits for three of them (TOI-5218b, TOI-5616b, TOI-5634Ab), while the fourth one—TOI-5414b is classified as a “likely planet.” Our observations include radial velocities from the Habitable-zone Planet Finder on the Hobby–Eberly Telescope, and MAROON-X on Gemini-North, along with photometry and high-contrast imaging from multiple ground-based facilities. In addition to TESS photometry, K2-419Ab was also observed and statistically validated as part of the K2 mission in Campaigns 5 and 18, which provide precise orbital and planetary constraints despite the faint host star and long orbital period of ∼20.4 days. With an equilibrium temperature of only 380 K, K2-419Ab is one of the coolest known well-characterized transiting planets. TOI-6034 has a late F-type companion about 40″ away, making it the first GEMS host star to have an earlier main-sequence binary companion. These confirmations add to the existing small sample of confirmed transiting GEMS.

The Astronomical JournalVol. 168(6)
National Science Foundation
Openalex Percentile: Top 7%
Stellar, planetary, and galactic studies
3.65
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