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Thermal Phase Curves of XO-3b: An Eccentric Hot Jupiter at the Deuterium Burning Limit
DOI: 10.3847/1538-3881/ac365f Bibcode: 2022AJ....163...32D

Deming, Drake; Burrows, Adam; Fortney, Jonathan J. +15 more

We report Spitzer full-orbit phase observations of the eccentric hot Jupiter XO-3b at 3.6 and 4.5 µm. Our new eclipse depth measurements of 1770 ± 180 ppm at 3.6 µm and 1610 ± 70 ppm at 4.5 µm show no evidence of the previously reported dayside temperature inversion. We also empirically derive the mass and radius of XO-3b and its…

2022 The Astronomical Journal
Gaia 10
The Transformative Journey of HD 93521
DOI: 10.3847/1538-3881/ac43be Bibcode: 2022AJ....163..100G

Gies, Douglas R.; Shepard, Katherine; Klement, Robert +1 more

HD 93521 is a massive, rapidly rotating star that is located about 1 kpc above the Galactic disk, and the evolutionary age for its estimated mass is much less than the time of flight if it was ejected from the disk. Here we present a reassessment of both the evolutionary and kinematical timescales for HD 93521. We calculate a time of flight of 39 …

2022 The Astronomical Journal
Gaia IUE eHST 10
Bayesian Inference in Single-line Spectroscopic Binaries with a Visual Orbit
DOI: 10.3847/1538-3881/ac5ab4 Bibcode: 2022AJ....163..220V

Mendez, Rene A.; Clavería, Rubén M.; Orchard, Marcos E. +2 more

We present a Bayesian inference methodology for the estimation of orbital parameters on single-line spectroscopic binaries with astrometric data, based on the No-U-Turn sampler Markov chain Monte Carlo algorithm. Our approach is designed to provide a precise and efficient estimation of the joint posterior distribution of the orbital parameters in …

2022 The Astronomical Journal
Gaia 10
A Spatially Dependent Correction of Gaia EDR3 Parallax Zero-point Offset based on 0.3 million LAMOST DR8 Giant Stars
DOI: 10.3847/1538-3881/ac4dec Bibcode: 2022AJ....163..149W

Huang, Yang; Yuan, Haibo; Wang, Chun

We have studied the zero-point offset of Gaia Early Data Release 3 (EDR3) parallaxes based on a sample of 0.3 million giant stars built from the LAMOST data with distance accuracy better than 8.5%. The official parallax zero-point corrections largely reduce the global offset in the Gaia EDR3 parallaxes: the global parallax offsets are -27.9 µ…

2022 The Astronomical Journal
Gaia 10
Hitting a New Low: The Unique 28 hr Cessation of Accretion in the TESS Light Curve of YY Dra (DO Dra)
DOI: 10.3847/1538-3881/ac5a51 Bibcode: 2022AJ....163..246H

Garnavich, Peter; Littlefield, Colin; Szkody, Paula +6 more

We present the Transiting Exoplanet Surveying Satellite light curve of the intermediate polar YY Draconis (YY Dra, also known as DO Dra). The power spectrum indicates that while there is stream-fed accretion for most of the observational period, there is a day-long, flat-bottomed low state at the beginning of 2020 during which the only periodic si…

2022 The Astronomical Journal
Gaia 9
Simultaneous Detection of Optical Flares of the Magnetically Active M-dwarf Wolf359
DOI: 10.3847/1538-3881/ac4e92 Bibcode: 2022AJ....163..164L

Wang, Shiang-Yu; Zhang, Yu; Lehner, Matthew J. +13 more

We present detections of stellar flares of Wolf 359, an M6.5 dwarf in the solar neighborhood (2.41 pc) known to be prone to flares due to surface magnetic activity. The observations were carried out from 2020 April 23 to 29 with a 1 m and a 0.5 m telescope separated by nearly 300 km in Xinjiang, China. In 27 hr of photometric monitoring, a total o…

2022 The Astronomical Journal
Gaia 9
Extremely Inclined Orbit of the S-type Planet γ Cep Ab Induced by the Eccentric Kozai-Lidov Mechanism
DOI: 10.3847/1538-3881/ac8f4c Bibcode: 2022AJ....164..177H

Ji, Jianghui; Huang, Xiumin

γ Cep Ab is a typical S-type planet, which occupies a nearly perpendicular planetary orbit relative to the binary. Here, we use a Markov Chain Monte Carlo sampler to conduct a full N-body fitting and derive self-consistent orbital solutions for this hierarchical system. We then employ the eccentric Kozai-Lidov (EKL) mechanism to explain the extrem…

2022 The Astronomical Journal
Gaia 9
A New Absolute Proper Motion Determination of Leo I Using HST/WFPC2 Images and Gaia EDR3
DOI: 10.3847/1538-3881/ac30dc Bibcode: 2022AJ....163....1C

Horch, Elliott P.; Kozhurina-Platais, Vera; Casetti-Dinescu, Dana I. +3 more

We measure the absolute proper motion of Leo I using a WFPC2/HST data set that spans up to 10 yr to date the longest time baseline utilized for this satellite. The measurement relies on ~2300 Leo I stars located near the center of light of the galaxy; the correction to absolute proper motion is based on 174 Gaia EDR3 stars and 10 galaxies. Having …

2022 The Astronomical Journal
Gaia eHST 9
The Galactic Distribution of Phosphorus: A Survey of 163 Disk and Halo Stars
DOI: 10.3847/1538-3881/ac77f8 Bibcode: 2022AJ....164...61M

Janowiecki, Steven; Cargile, Phillip; Hawkins, Keith +3 more

Phosphorus (P) is a critical element for life on Earth, yet the cosmic production sites of P are relatively uncertain. To understand how P has evolved in the solar neighborhood, we measured abundances for 163 FGK stars over a range of -1.09 < [Fe/H] < 0.47 using observations from the Habitable-zone Planet Finder instrument on the Hobby-Eberl…

2022 The Astronomical Journal
Gaia 9
A Mid-infrared Study of Directly Imaged Planetary-mass Companions Using Archival Spitzer/IRAC Images
DOI: 10.3847/1538-3881/ac3745 Bibcode: 2022AJ....163...36M

Kraus, Adam L.; Martinez, Raquel A.

The atmospheres and accretion disks of planetary-mass and substellar companions provide an unprecedented look into planet and moon formation processes, most notably the frequency and lifetime of circumplanetary disks. In our ongoing effort to leverage the extraordinary sensitivity of the Spitzer/Infrared Array Camera (IRAC) at 3.6, 4.5, 5.8, and 8…

2022 The Astronomical Journal
Gaia eHST 9