Search Publications

A Tendency Toward Alignment in Single-star Warm-Jupiter Systems
DOI: 10.3847/1538-3881/ac8153 Bibcode: 2022AJ....164..104R

Rice, Malena; Howard, Andrew W.; Dai, Fei +9 more

The distribution of spin-orbit angles for systems with wide-separation, tidally detached exoplanets offers a unique constraint on the prevalence of dynamically violent planetary evolution histories. Tidally detached planets provide a relatively unbiased view of the primordial stellar obliquity distribution, as they cannot tidally realign within th…

2022 The Astronomical Journal
Gaia 36
HATS-74Ab, HATS-75b, HATS-76b, and HATS-77b: Four Transiting Giant Planets Around K and M Dwarfs
DOI: 10.3847/1538-3881/ac4a77 Bibcode: 2022AJ....163..125J

Hobson, M.; Jordán, Andrés; Palle, E. +35 more

The relative rarity of giant planets around low-mass stars compared with solar-type stars is a key prediction from the core-accretion planet formation theory. In this paper we report on the discovery of four gas giant planets that transit low-mass late K and early M dwarfs. The planets HATS-74Ab (TOI 737b), HATS-75b (TOI 552b), HATS-76b (TOI 555b)…

2022 The Astronomical Journal
Gaia 35
Retrieving the C and O Abundances of HR 7672 AB: A Solar-type Primary Star with a Benchmark Brown Dwarf
DOI: 10.3847/1538-3881/ac56e2 Bibcode: 2022AJ....163..189W

Fitzgerald, Michael P.; Skemer, Andrew; Wallack, Nicole L. +30 more

A benchmark brown dwarf (BD) is a BD whose properties (e.g., mass and chemical composition) are precisely and independently measured. Benchmark BDs are valuable in testing theoretical evolutionary tracks, spectral synthesis, and atmospheric retrievals for substellar objects. Here, we report results of atmospheric retrieval on a synthetic spectrum …

2022 The Astronomical Journal
Gaia 34
A Possible Alignment Between the Orbits of Planetary Systems and their Visual Binary Companions
DOI: 10.3847/1538-3881/ac517f Bibcode: 2022AJ....163..207C

Vanderburg, Andrew; Bieryla, Allyson; Latham, David W. +111 more

Astronomers do not have a complete picture of the effects of wide-binary companions (semimajor axes greater than 100 au) on the formation and evolution of exoplanets. We investigate these effects using new data from Gaia Early Data Release 3 and the Transiting Exoplanet Survey Satellite mission to characterize wide-binary systems with transiting e…

2022 The Astronomical Journal
Gaia 34
Evidence that the Hot Jupiter WASP-77 A b Formed Beyond Its Parent Protoplanetary Disk's H2O Ice Line
DOI: 10.3847/1538-3881/ac4d9f Bibcode: 2022AJ....163..159R

Sing, David K.; Lothringer, Joshua D.; Reggiani, Henrique +2 more

Idealized protoplanetary disk and giant planet formation models have been interpreted to suggest that a giant planet's atmospheric abundances can be used to infer its formation location in its parent protoplanetary disk. It has recently been reported that the hot Jupiter WASP-77 A b has subsolar atmospheric carbon and oxygen abundances with a sola…

2022 The Astronomical Journal
Gaia 33
TOI-3714 b and TOI-3629 b: Two Gas Giants Transiting M Dwarfs Confirmed with the Habitable-zone Planet Finder and NEID
DOI: 10.3847/1538-3881/ac7804 Bibcode: 2022AJ....164...50C

Kobulnicky, Henry A.; Cochran, William D.; Mahadevan, Suvrath +36 more

We confirm the planetary nature of two gas giants discovered by the Transiting Exoplanet Survey Satellite to transit M dwarfs. TOI-3714 (V = 15.24, J = 11.74) is an M2 dwarf hosting a hot Jupiter (M p = 0.70 ± 0.03 M J and R p = 1.01 ± 0.03 R J ) on an orbital period of 2.154849 ± 0.000001 days wi…

2022 The Astronomical Journal
Gaia 33
The ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109
DOI: 10.3847/1538-3881/ac479d Bibcode: 2022AJ....163..114E

Fang, Min; Edwards, Suzan; Banzatti, Andrea +59 more

The Hubble UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Director's Discretionary Program of low-mass pre-main-sequence stars, coupled with forthcoming data from Atacama Large Millimeter/submillimeter Array and James Webb Space Telescope, will provide the foundation to revolutionize our understanding of the relationship between…

2022 The Astronomical Journal
Gaia eHST 31
Gemini-LIGHTS: Herbig Ae/Be and Massive T Tauri Protoplanetary Disks Imaged with Gemini Planet Imager
DOI: 10.3847/1538-3881/ac7be4 Bibcode: 2022AJ....164..109R

Monnier, John D.; Kraus, Stefan; Oppenheimer, Rebecca +20 more

We present the complete sample of protoplanetary disks from the Gemini- Large Imaging with the Gemini Planet Imager Herbig/T Tauri Survey, which observed bright Herbig Ae/Be stars and T Tauri stars in near-infrared polarized light to search for signatures of disk evolution and ongoing planet formation. The 44 targets were chosen based on their nea…

2022 The Astronomical Journal
Gaia 30
The K2-3 System Revisited: Testing Photoevaporation and Core-powered Mass Loss with Three Small Planets Spanning the Radius Valley
DOI: 10.3847/1538-3881/ac7807 Bibcode: 2022AJ....164..172D

Youngblood, Allison; Crossfield, Ian J. M.; Kreidberg, Laura +11 more

Multiplanet systems orbiting M dwarfs provide valuable tests of theories of small-planet formation and evolution. K2-3 is an early M dwarf hosting three small exoplanets (1.5-2.0 R ) at distances of 0.07-0.20 au. We measure the high-energy spectrum of K2-3 with HST/COS and XMM-Newton and use empirically driven estimates of Lyα and extr…

2022 The Astronomical Journal
Gaia XMM-Newton eHST 30
Dynamical Mass of the Young Substellar Companion HD 984 B
DOI: 10.3847/1538-3881/ac35e8 Bibcode: 2022AJ....163...50F

Dupuy, Trent J.; Kraus, Adam L.; Tran, Quang H. +5 more

Model-independent masses of substellar companions are critical tools to validate models of planet and brown dwarf cooling, test their input physics, and determine the formation and evolution of these objects. In this work, we measure the dynamical mass and orbit of the young substellar companion HD 984 B. We obtained new high-contrast imaging of t…

2022 The Astronomical Journal
Gaia Hipparcos 30