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Measuring Elemental Abundances of JWST Target Stars for Exoplanet Characterization. I. FGK Stars
DOI: 10.3847/1538-3881/ac7de3 Bibcode: 2022AJ....164...87K

Wang, Ji; Kolecki, Jared R.

With the launch of the JWST, we will obtain more precise data for exoplanets than ever before. However, these data can only inform and revolutionize our understanding of exoplanets when placed in the larger context of planet-star formation. Therefore, gaining a deeper understanding of their host stars is equally important and synergistic with the …

2022 The Astronomical Journal
Gaia 27
TOI-3757 b: A Low-density Gas Giant Orbiting a Solar-metallicity M Dwarf
DOI: 10.3847/1538-3881/ac7c20 Bibcode: 2022AJ....164...81K

Kobulnicky, Henry A.; Cochran, William D.; Mahadevan, Suvrath +32 more

We present the discovery of a new Jovian-sized planet, TOI-3757 b, the lowest-density transiting planet known to orbit an M dwarf (M0V). This planet was discovered around a solar-metallicity M dwarf, using Transiting Exoplanet Survey Satellite photometry and confirmed with precise radial velocities from the Habitable-zone Planet Finder (HPF) and N…

2022 The Astronomical Journal
Gaia 27
Bridging the Gap-The Disappearance of the Intermediate Period Gap for Fully Convective Stars, Uncovered by New ZTF Rotation Periods
DOI: 10.3847/1538-3881/ac9bee Bibcode: 2022AJ....164..251L

Angus, Ruth; Curtis, Jason L.; David, Trevor J. +2 more

The intermediate period gap, discovered by Kepler, is an observed dearth of stellar rotation periods in the temperature-period diagram at ~20 days for G dwarfs and up to ~30 days for early-M dwarfs. However, because Kepler mainly targeted solar-like stars, there is a lack of measured periods for M dwarfs, especially those at the fully convective l…

2022 The Astronomical Journal
Gaia 27
Roaring Storms in the Planetary-mass Companion VHS 1256-1257 b: Hubble Space Telescope Multiepoch Monitoring Reveals Vigorous Evolution in an Ultracool Atmosphere
DOI: 10.3847/1538-3881/ac9905 Bibcode: 2022AJ....164..239Z

Kataria, Tiffany; Apai, Dániel; Zhou, Yifan +5 more

The photometric and spectral variability of brown dwarfs probes heterogeneous temperature and cloud distributions and traces the atmospheric circulation patterns. We present a new 42 hr Hubble Space Telescope (HST) Wide Field Camera 3 G141 spectral time series of VHS 1256-1257 b, a late L-type planetary-mass companion that has been shown to have o…

2022 The Astronomical Journal
eHST 27
An Aligned Orbit for the Young Planet V1298 Tau b
DOI: 10.3847/1538-3881/ac6271 Bibcode: 2022AJ....163..247J

Berlind, Perry; Calkins, Michael L.; Esquerdo, Gilbert A. +22 more

The alignment of planetary orbits with respect to the stellar rotation preserves information on their dynamical histories. Measuring this angle for young planets helps illuminate the mechanisms that create misaligned orbits for older planets, as different processes could operate over timescales ranging from a few megayears to a gigayear. We presen…

2022 The Astronomical Journal
Gaia 26
Speckle Interferometry at SOAR in 2021
DOI: 10.3847/1538-3881/ac78e7 Bibcode: 2022AJ....164...58T

Tokovinin, Andrei; Mason, Brian D.; Mendez, Rene A. +1 more

The speckle interferometry program at the the 4.1 m Southern Astrophysical Research Telescope (SOAR), which started in 2008, now has accumulated over 30,300 individual observations of 12,700 distinct targets. Its main goal is to monitor orbital motion of close binaries, including members of high-order hierarchies and low-mass dwarfs in the solar n…

2022 The Astronomical Journal
Gaia Hipparcos 26
The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 Day Orbit with the Automated Planet Finder Telescope
DOI: 10.3847/1538-3881/ac415b Bibcode: 2022AJ....163...61D

Gagliano, Robert; Kristiansen, Martti H.; LaCourse, Daryll M. +72 more

We report the discovery of TOI-2180 b, a 2.8 M J giant planet orbiting a slightly evolved G5 host star. This planet transited only once in Cycle 2 of the primary Transiting Exoplanet Survey Satellite (TESS) mission. Citizen scientists identified the 24 hr single-transit event shortly after the data were released, allowing a Doppler moni…

2022 The Astronomical Journal
Gaia 25
The Solar Neighborhood. XLIX. New Discoveries and Orbits of M-dwarf Multiples with Speckle Interferometry at SOAR
DOI: 10.3847/1538-3881/ac52f6 Bibcode: 2022AJ....163..178V

Henry, Todd J.; Tokovinin, Andrei; Winters, Jennifer G. +3 more

We present the first results of a multiyear program to map the orbits of M-dwarf multiples within 25 pc. The observations were conducted primarily during 2019-2020 using speckle interferometry at the Southern Astrophysical Research Telescope in Chile, using the High-Resolution Camera mounted on the adaptive optics module (HRCam+SAM). The sample of…

2022 The Astronomical Journal
Gaia 25
Systematic KMTNet Planetary Anomaly Search. VI. Complete Sample of 2018 Sub-prime-field Planets
DOI: 10.3847/1538-3881/ac9c5c Bibcode: 2022AJ....164..262J

Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk +31 more

We complete the analysis of all 2018 sub-prime-field microlensing planets identified by the KMTNet AnomalyFinder. Among the 9 previously unpublished events with clear planetary solutions, 6 are clearly planetary (OGLE-2018-BLG-0298, KMT-2018-BLG-0087, KMT-2018-BLG-0247, KMT-2018-BLG-0030, OGLE-2018-BLG-1119, and KMT-2018-BLG-2602), while the remai…

2022 The Astronomical Journal
Gaia 25
Untangling the Galaxy. IV. Empirical Constraints on Angular Momentum Evolution and Gyrochronology for Young Stars in the Field
DOI: 10.3847/1538-3881/ac866d Bibcode: 2022AJ....164..137K

Stassun, Keivan G.; Kounkel, Marina; Bouma, Luke G. +3 more

We present a catalog of ~100,000 periodic variable stars in Transiting Exoplanet Survey Satellite (TESS) full-frame image data among members of widely distributed moving groups identified with Gaia in the previous papers in the series. By combining the periods from our catalog attributable to rotation with previously derived rotation periods for b…

2022 The Astronomical Journal
Gaia 25