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More Evidence for Variable Helium Absorption from HD 189733b
DOI: 10.3847/1538-3881/ac9675 Bibcode: 2022AJ....164..237Z

Redfield, Seth; Knutson, Heather A.; France, Kevin +5 more

We present a new Keck/NIRSPEC observation of metastable helium absorption from the upper atmosphere of HD 189733b, a hot Jupiter orbiting a nearby moderately active star. We measure an average helium transit depth of 0.420% ± 0.013% integrated over the [-20, 20] km s-1 velocity range. Comparing this measurement to eight previously publi…

2022 The Astronomical Journal
XMM-Newton 19
A Young, Low-density Stellar Stream in the Milky Way Disk: Theia 456
DOI: 10.3847/1538-3881/ac6952 Bibcode: 2022AJ....163..275A

Kounkel, Marina; Covey, Kevin R.; Agüeros, Marcel A. +4 more

Our view of the variety of stellar structures pervading the local Milky Way has been transformed by the application of clustering algorithms to the Gaia catalog. In particular, several stellar streams have been recently discovered that are comprised of hundreds to thousands of stars and span several hundred parsecs. We analyze one such structure, …

2022 The Astronomical Journal
Gaia 18
EXPRES. III. Revealing the Stellar Activity Radial Velocity Signature of ϵ Eridani with Photometry and Interferometry
DOI: 10.3847/1538-3881/ac3235 Bibcode: 2022AJ....163...19R

Monnier, John D.; Lanthermann, Cyprien; Anugu, Narsireddy +20 more

The distortions of absorption line profiles caused by photospheric brightness variations on the surfaces of cool, main-sequence stars can mimic or overwhelm radial velocity (RV) shifts due to the presence of exoplanets. The latest generation of precision RV spectrographs aims to detect velocity amplitudes ≲ 10 cm s-1, but requires mitig…

2022 The Astronomical Journal
Gaia 18
Planets Across Space and Time (PAST). III. Morphology of the Planetary Radius Valley as a Function of Stellar Age and Metallicity in the Galactic Context Revealed by the LAMOST-Gaia-Kepler Sample
DOI: 10.3847/1538-3881/ac641f Bibcode: 2022AJ....163..249C

Dong, Subo; Zong, Weikai; Zhu, Zi +7 more

The radius valley, a dip in the radius distribution of exoplanets at ~1.9 R , separates compact rocky super-Earths and sub-Neptunes with lower density. Various hypotheses have been put forward to explain the radius valley. Characterizing the radius valley morphology and its correlation to stellar properties will provide crucial observa…

2022 The Astronomical Journal
Gaia 18
A Mini-Neptune from TESS and CHEOPS Around the 120 Myr Old AB Dor Member HIP 94235
DOI: 10.3847/1538-3881/ac69e3 Bibcode: 2022AJ....163..289Z

Latham, David W.; Quinn, Samuel N.; Kane, Stephen R. +36 more

The Transiting Exoplanet Survey Satellite (TESS) mission has enabled discoveries of the brightest transiting planet systems around young stars. These systems are the benchmarks for testing theories of planetary evolution. We report the discovery of a mini-Neptune transiting a bright star in the AB Doradus moving group. HIP 94235 (TOI-4399, TIC 464…

2022 The Astronomical Journal
CHEOPS Gaia Hipparcos 18
The Open Cluster Chemical Abundances and Mapping Survey. VII. APOGEE DR17 [C/N]-Age Calibration
DOI: 10.3847/1538-3881/ac5d53 Bibcode: 2022AJ....163..229S

Bizyaev, Dmitry; Pan, Kaike; Cunha, Katia +11 more

Large-scale surveys open the possibility to investigate Galactic evolution both chemically and kinematically; however, reliable stellar ages remain a major challenge. Detailed chemical information provided by high-resolution spectroscopic surveys of the stars in clusters can be used as a means to calibrate recently developed chemical tools for age…

2022 The Astronomical Journal
Gaia 18
Orbital Elements and Individual Component Masses from Joint Spectroscopic and Astrometric Data of Double-line Spectroscopic Binaries
DOI: 10.3847/1538-3881/ac478c Bibcode: 2022AJ....163..118A

Anguita-Aguero, Jennifer; Mendez, Rene A.; Clavería, Rubén M. +1 more

We present orbital elements, orbital parallaxes, and individual component masses for 14 spatially resolved double-line spectroscopic binaries derived doing a simultaneous fit of their visual orbit and radial velocity curve. This was done by means of a Markov Chain Monte Carlo code developed by our group that produces posterior distribution functio…

2022 The Astronomical Journal
Gaia Hipparcos 18
Revisiting KELT-19Ab, WASP-156b, and WASP-121b in the TESS Era
DOI: 10.3847/1538-3881/ac3b4e Bibcode: 2022AJ....163...42Y

Chary, Ranga-Ram; Yang, Fan; Liu, Ji-Feng

We present a re-analysis of transit depths of KELT-19Ab, WASP-156b, and WASP-121b, including data from the Transiting Exoplanet Survey Satellite (TESS). The large ~21″ TESS pixels and point-spread function result in significant contamination of the stellar flux by nearby objects. We use Gaia data to fit for and remove this contribution, providing …

2022 The Astronomical Journal
Gaia eHST 17
Inhomogeneity within Local Interstellar Clouds
DOI: 10.3847/1538-3881/ac816b Bibcode: 2022AJ....164..106L

Redfield, Seth; Linsky, Jeffrey L.; Ryder, Diana +1 more

Analysis of interstellar absorption lines observed in high-resolution Hubble Space Telescope spectra of nearby stars provides temperatures, turbulent velocities, and kinetic properties of warm interstellar clouds. A new analysis of 97 interstellar-velocity components reveals a wide range of temperatures and turbulent velocities within the Local In…

2022 The Astronomical Journal
Ulysses eHST 17
Dynamical Mass of the Exoplanet Host Star HR 8799
DOI: 10.3847/1538-3881/ac3bb5 Bibcode: 2022AJ....163...52S

Bowler, Brendan P.; Sepulveda, Aldo G.

HR 8799 is a young A5/F0 star hosting four directly imaged giant planets at wide separations (~16-78 au), which are undergoing orbital motion and have been continuously monitored with adaptive optics imaging since their discovery over a decade ago. We present a dynamical mass of HR 8799 using 130 epochs of relative astrometry of its planets, which…

2022 The Astronomical Journal
Gaia eHST 17