Search Publications

The Rapid Rotation of the Strongly Magnetic Ultramassive White Dwarf EGGR 156
DOI: 10.3847/1538-3881/ac8543 Bibcode: 2022AJ....164..131W

Hermes, J. J.; Vanderbosch, Zachary P.; Williams, Kurtis A.

The distribution of white dwarf rotation periods provides a means for constraining angular momentum evolution during the late stages of stellar evolution, as well as insight into the physics and remnants of double degenerate mergers. Although the rotational distribution of low-mass white dwarfs is relatively well constrained via asteroseismology, …

2022 The Astronomical Journal
Gaia 15
HD-TESS: An Asteroseismic Catalog of Bright Red Giants within TESS Continuous Viewing Zones
DOI: 10.3847/1538-3881/ac8931 Bibcode: 2022AJ....164..135H

Huber, Daniel; Stello, Dennis; Hon, Marc +2 more

We present HD-TESS, a catalog of 1709 bright (V ~ 3-10) red giants from the Henry Draper (HD) Catalog with asteroseismic measurements based on photometry from NASA's Transiting Exoplanet Survey Satellite (TESS). Using light curves spanning at least 6 months across a single TESS observing cycle, we provide measurements of global asteroseismic param…

2022 The Astronomical Journal
Gaia 15
The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age
DOI: 10.3847/1538-3881/ac5324 Bibcode: 2022AJ....163..166Q

Williams, Benjamin F.; Gilbert, Karoline M.; Chemin, Laurent +8 more

Triangulum (M33) is a low-mass, relatively undisturbed spiral galaxy that offers a new regime in which to test models of dynamical heating. In spite of its proximity, M33's dynamical heating history has not yet been well-constrained. In this work, we present the TREX Survey, the largest stellar spectroscopic survey across the disk of M33. We prese…

2022 The Astronomical Journal
eHST 15
Detection of Near-infrared Water Ice at the Surface of the (Pre)Transitional Disk of AB Aur: Informing Icy Grain Abundance, Composition, and Size
DOI: 10.3847/1538-3881/ac4d9b Bibcode: 2022AJ....163..145B

Pinte, C.; Ménard, F.; Duchêne, G. +17 more

We present near-infrared Large Binocular Telescope LMIRCam imagery of the disk around the Herbig Ae/Be star AB Aurigae. A comparison of the surface brightness at K s (2.16 µm), H2O narrowband (3.08 µm), and $L^{\prime} $ (3.7 µm) allows us to probe the presence of icy grains in this (pre)transitional disk …

2022 The Astronomical Journal
ISO 15
Automatic Morphological Classification of Galaxies: Convolutional Autoencoder and Bagging-based Multiclustering Model
DOI: 10.3847/1538-3881/ac4245 Bibcode: 2022AJ....163...86Z

Fang, Guanwen; Lin, Zesen; Gu, Yizhou +1 more

In order to obtain morphological information of unlabeled galaxies, we present an unsupervised machine-learning (UML) method for morphological classification of galaxies, which can be summarized as two aspects: (1) the methodology of convolutional autoencoder (CAE) is used to reduce the dimensions and extract features from the imaging data; (2) th…

2022 The Astronomical Journal
eHST 15
Correcting Stellar Flare Frequency Distributions Detected by TESS and Kepler
DOI: 10.3847/1538-3881/ac937e Bibcode: 2022AJ....164..213G

Yang, Ming; Zhou, Ji-Lin; Liu, Hui-Gen +1 more

The habitability of planets is closely connected with stellar activity, mainly the frequency of flares and the distribution of flare energy. Kepler and TESS find many flaring stars via precise time-domain photometric data, and the frequency and energy distribution of stellar flares on different types of stars are studied statistically. However, th…

2022 The Astronomical Journal
Gaia 15
A Dearth of Close-in Stellar Companions to M-dwarf TESS Objects of Interest
DOI: 10.3847/1538-3881/ac6101 Bibcode: 2022AJ....163..232C

Howell, Steve B.; Beichman, Charles A.; Ciardi, David R. +5 more

TESS has proven to be a powerful resource for finding planets, including those that orbit the most prevalent stars in our galaxy: M dwarfs. Identification of stellar companions (both bound and unbound) has become a standard component of the transiting planet confirmation process in order to assess the level of light-curve dilution and the possibil…

2022 The Astronomical Journal
Gaia 15
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