Search Publications

Untangling the Galaxy. III. Photometric Search for Pre-main-sequence Stars with Deep Learning
DOI: 10.3847/1538-3881/ac2432 Bibcode: 2021AJ....162..282M

Kounkel, Marina; Covey, Kevin; Hutchinson, Brian +2 more

A reliable census of pre-main-sequence stars with known ages is critical to our understanding of early stellar evolution, but historically there has been difficulty in separating such stars from the field. We present a trained neural network model, Sagitta, that relies on Gaia DR2 and 2 Micron All-Sky Survey photometry to identify pre-main-sequenc…

2021 The Astronomical Journal
Gaia 31
A Uniform Search for Nearby Planetary Companions to Hot Jupiters in TESS Data Reveals Hot Jupiters Are Still Lonely
DOI: 10.3847/1538-3881/ac2602 Bibcode: 2021AJ....162..263H

Barclay, Thomas; Wohler, Bill; Ricker, George R. +12 more

We present the results of a uniform search for additional planets around all stars with confirmed hot Jupiters observed by the Transiting Exoplanet Survey Satellite (TESS) in its Cycle 1 survey of the southern ecliptic hemisphere. Our search comprises 184 total planetary systems with confirmed hot Jupiters with R p > 8 R

2021 The Astronomical Journal
Gaia 30
TOI-1278 B: SPIRou Unveils a Rare Brown Dwarf Companion in Close-in Orbit around an M Dwarf
DOI: 10.3847/1538-3881/ac096d Bibcode: 2021AJ....162..144A

Torres, Guillermo; Latham, David W.; Seager, Sara +39 more

We present the discovery of an 18.5 ± 0.5 MJup brown dwarf (BD) companion to the M0V star TOI-1278. The system was first identified through a percent-deep transit in Transiting Exoplanet Survey Satellite photometry; further analysis showed it to be a grazing transit of a Jupiter-sized object. Radial velocity (RV) follow-up with the SPIR…

2021 The Astronomical Journal
Gaia 30
The ZTF Source Classification Project. I. Methods and Infrastructure
DOI: 10.3847/1538-3881/abe853 Bibcode: 2021AJ....161..267V

Kulkarni, S. R.; Duev, Dmitry A.; Riddle, Reed +22 more

The Zwicky Transient Facility (ZTF) has been observing the entire northern sky since the start of 2018 down to a magnitude of 20.5 (5σ for 30 s exposure) in the g, r, and i filters. Over the course of two years, ZTF has obtained light curves of more than a billion sources, each with 50-1000 epochs per light curve in g and r, and fewer in i. To be …

2021 The Astronomical Journal
Gaia 30
TESS Data for Asteroseismology: Photometry
DOI: 10.3847/1538-3881/ac09f1 Bibcode: 2021AJ....162..170H

Huber, Daniel; Jenkins, Jon M.; Pope, Benjamin J. S. +12 more

Over the last two decades, asteroseismology has increasingly proven to be the observational tool of choice for the study of stellar physics, aided by the high quality of data available from space-based missions such as CoRoT, Kepler, K2, and the Transiting Exoplanet Survey Satellite (TESS). TESS in particular will produce more than an order of mag…

2021 The Astronomical Journal
Gaia 29
TOI-1634 b: An Ultra-short-period Keystone Planet Sitting inside the M-dwarf Radius Valley
DOI: 10.3847/1538-3881/ac0157 Bibcode: 2021AJ....162...79C

López-Morales, Mercedes; Bieryla, Allyson; Latham, David W. +63 more

Studies of close-in planets orbiting M dwarfs have suggested that the M-dwarf radius valley may be well explained by distinct formation timescales between enveloped terrestrials and rocky planets that form at late times in a gas-depleted environment. This scenario is at odds with the picture that close-in rocky planets form with a primordial gaseo…

2021 The Astronomical Journal
Gaia 29
Obliquity Constraints on the Planetary-mass Companion HD 106906 b
DOI: 10.3847/1538-3881/ac1bb1 Bibcode: 2021AJ....162..217B

Morley, Caroline V.; Bowler, Brendan P.; Bryan, Marta L. +2 more

We constrain the angular momentum architecture of HD 106906, a 13 ± 2 Myr old system in the ScoCen complex composed of a compact central binary, a widely separated planetary-mass tertiary HD 106906 b, and a debris disk nested between the binary and tertiary orbital planes. We measure the orientations of three vectors: the companion spin axis, comp…

2021 The Astronomical Journal
eHST 29
Constraining the Orbit and Mass of epsilon Eridani b with Radial Velocities, Hipparcos IAD-Gaia DR2 Astrometry, and Multiepoch Vortex Coronagraphy Upper Limits
DOI: 10.3847/1538-3881/ac134a Bibcode: 2021AJ....162..181L

Rice, Malena; Rosenthal, Lee J.; Hirsch, Lea A. +30 more

ϵ Eridani is a young planetary system hosting a complex multibelt debris disk and a confirmed Jupiter-like planet orbiting at 3.48 au from its host star. Its age and architecture are thus reminiscent of the early Solar System. The most recent study of Mawet et al., which combined radial-velocity data and Ms-band direct imaging upper limits, starte…

2021 The Astronomical Journal
Gaia Hipparcos 28
Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths with Earth-like Compositions
DOI: 10.3847/1538-3881/ac0fdc Bibcode: 2021AJ....162..161H

Barclay, Thomas; Vanderburg, Andrew; Bieryla, Allyson +60 more

We present observations of two bright M dwarfs (TOI-1634 and TOI-1685: J = 9.5-9.6) hosting ultra-short-period (USP) planets identified by the TESS mission. The two stars are similar in temperature, mass, and radius (Teff ≈ 3500 K, M ≈ 0.45-0.46 M, and R ≈ 0.45-0.46 R), and the planets are…

2021 The Astronomical Journal
Gaia 28
htof: A New Open-source Tool for Analyzing Hipparcos, Gaia, and Future Astrometric Missions
DOI: 10.3847/1538-3881/ac12d0 Bibcode: 2021AJ....162..230B

Dupuy, Trent J.; Brandt, Timothy D.; Li, Yiting +3 more

We present htof, an open-source tool for interpreting and fitting the intermediate astrometric data (IAD) from both the 1997 and 2007 reductions of Hipparcos, the scanning law of Gaia, and future missions such as the Nancy Grace Roman Space Telescope (NGRST). htof solves the astrometric parameters of any system for any arbitrary combination of abs…

2021 The Astronomical Journal
Gaia Hipparcos 28