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A Census of the 32 Ori Association with Gaia
DOI: 10.3847/1538-3881/ac85e2 Bibcode: 2022AJ....164..151L

Luhman, K. L.

I have used high-precision photometry and astrometry from the third data release of Gaia (DR3) to identify candidate members of the 32 Ori association. Spectral types and radial velocities have been measured for subsets of the candidates using new and archival spectra. For the candidates that have radial velocity measurements, I have used UVW velo…

2022 The Astronomical Journal
Gaia 15
HST/WFC3 Complete Phase-resolved Spectroscopy of White-dwarf-brown-dwarf Binaries WD 0137 and EPIC 2122
DOI: 10.3847/1538-3881/ac3095 Bibcode: 2022AJ....163...17Z

Mayorga, L. C.; Lothringer, Joshua D.; Apai, Dániel +7 more

Brown dwarfs in close-in orbits around white dwarfs offer an excellent opportunity to investigate properties of fast-rotating, tidally locked, and highly irradiated atmospheres. We present Hubble Space Telescope Wide Field Camera 3 G141 phase-resolved observations of two brown-dwarf-white-dwarf binaries: WD 0137-349 and EPIC 212235321. Their 1.1-1…

2022 The Astronomical Journal
Gaia eHST 14
Sensitive Multibeam Targeted SETI Observations toward 33 Exoplanet Systems with FAST
DOI: 10.3847/1538-3881/ac8bd5 Bibcode: 2022AJ....164..160T

Zhu, Yan; Li, Di; Qian, Lei +19 more

As a major approach to looking for life beyond the Earth, the search for extraterrestrial intelligence (SETI) is committed to searching for technosignatures such as engineered radio signals that are indicative of technologically capable life. In this paper, we report a targeted SETI campaign employing an observation strategy named multibeam coinci…

2022 The Astronomical Journal
Gaia 14
A Pilot Radio Search for Magnetic Activity in Directly Imaged Exoplanets
DOI: 10.3847/1538-3881/ac32c8 Bibcode: 2022AJ....163...15C

Berger, E.; Cendes, Y.; Williams, P. K. G.

We present the first systematic search for GHz frequency radio emission from directly imaged exoplanets using Very Large Array observations of sufficient angular resolution to separate the planets from their host stars. We obtained results for five systems and eight exoplanets located at ≲50 pc through new observations (Ross 458, GU Psc, and 51 Er…

2022 The Astronomical Journal
eHST 14
Hubble WFC3 Spectroscopy of the Rocky Planet L 98-59 b: No Evidence for a Cloud-free Primordial Atmosphere
DOI: 10.3847/1538-3881/ac8fe9 Bibcode: 2022AJ....164..203Z

Wang, Yonghao; Zhou, Li; Ma, Bo +1 more

We are using archived data from HST of transiting exoplanet L 98-59 b to place constraints on its potentially hot atmosphere. We analyze the data from five transit visits and extract the final combined transmission spectrum using Iraclis. Then we use the inverse atmospheric retrieval code TauREx to analyze the combined transmission spectrum. There…

2022 The Astronomical Journal
eHST 14
Deep Generative Modeling of Periodic Variable Stars Using Physical Parameters
DOI: 10.3847/1538-3881/ac9b3f Bibcode: 2022AJ....164..263M

Bloom, Joshua S.; Martínez-Palomera, Jorge; Abrahams, Ellianna S.

The ability to generate physically plausible ensembles of variable sources is critical to the optimization of time domain survey cadences and the training of classification models on data sets with few to no labels. Traditional data augmentation techniques expand training sets by reenvisioning observed exemplars, seeking to simulate observations o…

2022 The Astronomical Journal
Gaia 14
The Hubble PanCET Program: A Featureless Transmission Spectrum for WASP-29b and Evidence of Enhanced Atmospheric Metallicity on WASP-80b
DOI: 10.3847/1538-3881/ac7234 Bibcode: 2022AJ....164...30W

Deming, Drake; Mikal-Evans, Thomas; Sing, David K. +19 more

We present a uniform analysis of transit observations from the Hubble Space Telescope and Spitzer Space Telescope of two warm gas giants orbiting K-type stars-WASP-29b and WASP-80b. The transmission spectra, which span 0.4-5.0 µm, are interpreted using a suite of chemical equilibrium PLATON atmospheric retrievals. Both planets show evidence …

2022 The Astronomical Journal
Gaia XMM-Newton eHST 13
KELT-9 as an Eclipsing Double-lined Spectroscopic Binary: A Unique and Self-consistent Solution to the System
DOI: 10.3847/1538-3881/ac32c7 Bibcode: 2022AJ....163...40P

Gaudi, B. Scott; Eastman, Jason D.; Wang, Ji +5 more

Transiting hot Jupiters present a unique opportunity to measure absolute planetary masses due to the magnitude of their radial velocity signals and known orbital inclination. Measuring planet mass is critical to understanding atmospheric dynamics and escape under extreme stellar irradiation. Here we present the ultrahot Jupiter system KELT-9 as a …

2022 The Astronomical Journal
Gaia 13
A Gaia View on the Star Formation in the Monoceros OB1 and R1 Associations
DOI: 10.3847/1538-3881/ac63b6 Bibcode: 2022AJ....163..266L

Lim, Beomdu; Lee, Jeong-Eun; Park, Byeong-Gon +5 more

Stellar kinematics provides the key to understanding the star formation process. In this respect, we present a kinematic study of the Monoceros OB1 (Mon OB1) and R1 (Mon R1) associations using the recent Gaia data and radial velocities of stars derived from high-resolution spectroscopy and the literature. A total of 728 members are selected using …

2022 The Astronomical Journal
AKARI Gaia 13
The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets
DOI: 10.3847/1538-3881/ac3a06 Bibcode: 2022AJ....163..128W

Cunha, Katia; Smith, Verne V.; Mahadevan, Suvrath +15 more

The chemical abundances of planet-hosting stars offer a glimpse into the composition of planet-forming environments. To further understand this connection, we make the first ever measurement of the correlation between planet occurrence and chemical abundances for ten different elements (C, Mg, Al, Si, S, K, Ca, Mn, Fe, and Ni). Leveraging data fro…

2022 The Astronomical Journal
Gaia 13