Search Publications

The Stellar Velocity Distribution Function in the Milky Way Galaxy
DOI: 10.3847/1538-3881/ab9813 Bibcode: 2020AJ....160...43A

Majewski, Steven R.; Beers, Timothy C.; Hayes, Christian R. +6 more

The stellar velocity distribution function in the solar vicinity is reexamined using data from the Sloan Digital Sky Survey Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey's DR16 and Gaia DR2. By exploiting APOGEE's ability to chemically discriminate with great reliability the thin-disk, thick-disk, and (accreted) halo popul…

2020 The Astronomical Journal
Gaia 31
Exploring the Mass-loss Histories of the Red Supergiants
DOI: 10.3847/1538-3881/abab15 Bibcode: 2020AJ....160..145H

Humphreys, Roberta M.; Jones, Terry J.; Gordon, Michael S. +1 more

We report mid- to far-infrared imaging and photometry from 7 to 37 µm with SOFIA/FORCAST and 2 µm adaptive optics imaging with LBTI/LMIRCam of a large sample of red supergiants (RSGs) in four Galactic clusters: RSGC1, RSGC2 = Stephenson 2, RSGC3, and NGC 7419. The RSGs in these clusters cover their expected range in luminosity and init…

2020 The Astronomical Journal
AKARI 31
Transits of Known Planets Orbiting a Naked-eye Star
DOI: 10.3847/1538-3881/aba835 Bibcode: 2020AJ....160..129K

Butler, R. Paul; Kristiansen, Martti H.; Vanderburg, Andrew +45 more

Some of the most scientifically valuable transiting planets are those that were already known from radial velocity (RV) surveys. This is primarily because their orbits are well characterized and they preferentially orbit bright stars that are the targets of RV surveys. The Transiting Exoplanet Survey Satellite (TESS) provides an opportunity to sur…

2020 The Astronomical Journal
Gaia 30
Moderate-resolution K-band Spectroscopy of Substellar Companion κ Andromedae b
DOI: 10.3847/1538-3881/abb9b1 Bibcode: 2020AJ....160..207W

Macintosh, Bruce; Barman, Travis S.; Marois, Christian +5 more

We present moderate-resolution (R ∼ 4000) K-band spectra of the "super-Jupiter," κ Andromedae b. The data were taken with the OSIRIS integral field spectrograph at Keck Observatory. The spectra reveal resolved molecular lines from H2O and CO, and are compared to a custom PHOENIX atmosphere model grid appropriate for young planetary-mass…

2020 The Astronomical Journal
Gaia 30
An Updated Visual Orbit of the Directly Imaged Exoplanet 51 Eridani b and Prospects for a Dynamical Mass Measurement with Gaia
DOI: 10.3847/1538-3881/ab4da4 Bibcode: 2020AJ....159....1D

Duchêne, Gaspard; Esposito, Thomas M.; Hom, Justin +51 more

We present a revision to the visual orbit of the young, directly imaged exoplanet 51 Eridani b using four years of observations with the Gemini Planet Imager. The relative astrometry is consistent with an eccentric (e={0.53}-0.13+0.09) orbit at an intermediate inclination (i={136}-11+10 °), although circ…

2020 The Astronomical Journal
Gaia Hipparcos 30
KELT-11 b: Abundances of Water and Constraints on Carbon-bearing Molecules from the Hubble Transmission Spectrum
DOI: 10.3847/1538-3881/abbe12 Bibcode: 2020AJ....160..260C

Tsiaras, A.; Waldmann, I. P.; Tinetti, G. +4 more

In the past decade, the analysis of exoplanet atmospheric spectra has revealed the presence of water vapor in almost all the planets observed, with the exception of a fraction of overcast planets. Indeed, water vapor presents a large absorption signature in the wavelength coverage of the Hubble Space Telescope's (HST) Wide Field Camera 3 (WFC3), w…

2020 The Astronomical Journal
eHST 30
HATS-71b: A Giant Planet Transiting an M3 Dwarf Star in TESS Sector 1
DOI: 10.3847/1538-3881/ab8ad1 Bibcode: 2020AJ....159..267B

Kim, J.; Butler, R. P.; Winn, J. N. +41 more

We report the discovery of HATS-71b, a transiting gas giant planet on a $P=3.7955$ day orbit around a $G=15.35$ mag M3 dwarf star. HATS-71 is the coolest M dwarf star known to host a hot Jupiter. The loss of light during transits is 4.7%, more than in any other confirmed transiting planet system. The planet was identified as a candidate by the gro…

2020 The Astronomical Journal
Gaia 30
An Investigation of Poorly Studied Open Cluster NGC 4337 Using Multicolor Photometric and Gaia DR2 Astrometric Data
DOI: 10.3847/1538-3881/ab9ffd Bibcode: 2020AJ....160..119B

Bisht, D.; Rangwal, Geeta; Yadav, R. K. S. +5 more

We present a comprehensive analysis (photometric and kinematical) of the poorly studied open cluster NGC 4337 using 2MASS, WISE, APASS, and Gaia DR2 databases. By determining the membership probabilities of stars, we identified the 624 most probable members with membership probability higher than 50% by using proper motion and parallax data taken …

2020 The Astronomical Journal
Gaia 30
TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet
DOI: 10.3847/1538-3881/ab9f95 Bibcode: 2020AJ....160...96T

Butler, R. Paul; Torres, Guillermo; Barclay, Thomas +44 more

The Transiting Exoplanet Survey Satellite mission was designed to find transiting planets around bright, nearby stars. Here, we present the detection and mass measurement of a small, short-period (≈4 days) transiting planet around the bright (V = 7.9), solar-type star HD 86226 (TOI-652, TIC 22221375), previously known to host a long-period (∼1600 …

2020 The Astronomical Journal
Gaia 29
Loose Ends for the Exomoon Candidate Host Kepler-1625b
DOI: 10.3847/1538-3881/ab7001 Bibcode: 2020AJ....159..142T

Angus, Ruth; Howard, Andrew W.; Kipping, David +2 more

The claim of an exomoon candidate in the Kepler-1625b system has generated substantial discussion regarding possible alternative explanations for the purported signal. In this work, we examine these possibilities in detail. First, the effect of more flexible trend models is explored, and we show that sufficiently flexible models are capable of att…

2020 The Astronomical Journal
eHST 29