Search Publications

Planetary Candidates from K2 Campaign 16
DOI: 10.3847/1538-3881/aac6e6 Bibcode: 2018AJ....156...22Y

Henning, Thomas; Schlieder, Joshua E.; Fulton, Benjamin J. +20 more

Given that Campaign 16 of the K2 mission is one of just two K2 campaigns observed so far in “forward-facing” mode, which enables immediate follow-up observations from the ground, we present a catalog of interesting targets identified through photometry alone. Our catalog includes 30 high-quality planet candidates (showing no signs of being non-pla…

2018 The Astronomical Journal
Gaia 34
Direct Imaging of the HD 35841 Debris Disk: A Polarized Dust Ring from Gemini Planet Imager and an Outer Halo from HST/STIS
DOI: 10.3847/1538-3881/aacbc9 Bibcode: 2018AJ....156...47E

Duchêne, Gaspard; Esposito, Thomas M.; Oppenheimer, Rebecca +55 more

We present new high resolution imaging of a light-scattering dust ring and halo around the young star HD 35841. Using spectroscopic and polarimetric data from the Gemini Planet Imager in H-band (1.6 µm), we detect the highly inclined (i = 85°) ring of debris down to a projected separation of ∼12 au (∼0.″12) for the first time. Optical imagin…

2018 The Astronomical Journal
Gaia eHST 33
Discovery of a Transiting Adolescent Sub-Neptune Exoplanet with K2
DOI: 10.3847/1538-3881/aaeed7 Bibcode: 2018AJ....156..302D

Vanderburg, Andrew; Bieryla, Allyson; Latham, David W. +19 more

The role of stellar age in the measured properties and occurrence rates of exoplanets is not well understood. This is in part due to a paucity of known young planets and the uncertainties in age-dating for most exoplanet host stars. Exoplanets with well-constrained ages, particularly those which are young, are useful as benchmarks for studies aimi…

2018 The Astronomical Journal
Gaia 33
The Gas Composition and Deep Cloud Structure of Jupiter's Great Red Spot
DOI: 10.3847/1538-3881/aad186 Bibcode: 2018AJ....156..101B

Wong, M. H.; Orton, G. S.; de Pater, I. +3 more

We have obtained high-resolution spectra of Jupiter’s Great Red Spot (GRS) between 4.6-5.4 µm using telescopes on Mauna Kea to derive gas abundances and to constrain its cloud structure between 0.5-5 bars. We used line profiles of deuterated methane (CH3D) at 4.66 µm to infer the presence of an opaque cloud at 5 ± 1 bars. Fr…

2018 The Astronomical Journal
eHST 33
The Warm Neptunes around HD 106315 Have Low Stellar Obliquities
DOI: 10.3847/1538-3881/aad085 Bibcode: 2018AJ....156...93Z

Vanderburg, Andrew; Bieryla, Allyson; Latham, David W. +8 more

We present the obliquity of the warm Neptune HD 106315c measured via a series of spectroscopic transit observations. HD 106315c is a 4.4 R Earth warm Neptune orbiting a moderately rotating late F star with a period of 21.05 days. HD 106315 also hosts a 2.5 R Earth super-Earth on a 9.55 day orbit. Our Doppler tomographic analy…

2018 The Astronomical Journal
Gaia 32
Fundamental Properties of Co-moving Stars Observed by Gaia
DOI: 10.3847/1538-3881/aaaebe Bibcode: 2018AJ....155..149B

Faherty, Jacqueline K.; Gagné, Jonathan; Bochanski, John J. +5 more

We have estimated fundamental parameters for a sample of co-moving stars observed by Gaia and identified by Oh et al. We matched the Gaia observations to the 2MASS and Wide-Field Infrared Survey Explorer catalogs and fit MIST isochrones to the data, deriving estimates of the mass, radius, [Fe/H], age, distance, and extinction to 9754 stars in the …

2018 The Astronomical Journal
Gaia 32
Memberships of the Open Cluster NGC 6405 Based on a Combined Method: Gaussian Mixture Model and Random Forest
DOI: 10.3847/1538-3881/aad690 Bibcode: 2018AJ....156..121G

Gao, Xinhua

This paper presents a combined method of Gaussian mixture model and random forest to compute membership probabilities of stars by using large, high-dimensional data sets. A significant advantage of this method is that it allows us to easily identify likely cluster members in large data sets starting from small training samples. As a benchmark, we …

2018 The Astronomical Journal
Gaia 32
Four New Eclipsing Mid M-dwarf Systems from the New Luyten Two Tenths Catalog
DOI: 10.3847/1538-3881/aad9a3 Bibcode: 2018AJ....156..140I

Latham, David W.; Berlind, Perry; Calkins, Michael L. +7 more

Using data from the MEarth-North and MEarth-South transit surveys, we present the detection of eclipses in four mid M-dwarf systems: LP 107-25, LP 261-75, LP 796-24, and LP 991-15. Combining the MEarth photometry with spectroscopic follow-up observations, we show that LP 107-25 and LP 796-24 are short-period (1.388 and 0.523 day, respectively) ecl…

2018 The Astronomical Journal
Gaia 32
The Hawaii Infrared Parallax Program. III. 2MASS J0249-0557 c: A Wide Planetary-mass Companion to a Low-mass Binary in the β Pic Moving Group
DOI: 10.3847/1538-3881/aacbc2 Bibcode: 2018AJ....156...57D

Kratter, Kaitlin M.; Dupuy, Trent J.; Kraus, Adam L. +6 more

We have discovered a wide planetary-mass companion to the β Pic moving group member 2MASS J02495639-0557352 (M6 VL-G) using Canada-France-Hawaii Telescope/WIRCam astrometry from the Hawaii Infrared Parallax Program. In addition, Keck laser guide star adaptive optics aperture-masking interferometry shows that the host is itself a tight binary. Alto…

2018 The Astronomical Journal
Gaia 32
First Data Release of the All-sky NOAO Source Catalog
DOI: 10.3847/1538-3881/aad68f Bibcode: 2018AJ....156..131N

Nidever, David L.; Olsen, Knut; Dey, Arjun +6 more

Most of the sky has been imaged with NOAO’s telescopes from both hemispheres. While the large majority of these data were obtained for PI-led projects and almost all of the images are publicly available, only a small fraction have been released to the community via well-calibrated and easily accessible catalogs. We are remedying this by creating a…

2018 The Astronomical Journal
Gaia 32