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20112026
most citedAn Excess of Jupiter Analogs in Super-Earth Systems

190 citations · 1.8k across the 42 of their papers we have counts for

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Showing 2024Show all

7 papers · 1 filter

astro-ph.EP2024★ 17 cited

Leaning Sideways: VHS 1256-1257 b is a Super-Jupiter with a Uranus-like Obliquity

Michael Poon, Marta L. Bryan, Hanno Rein +4

We constrain the angular momentum architecture of VHS J125601.92-125723.9, a 140 20 Myr old hierarchical triple system composed of a low-mass binary and a widely-separated pl…

astro-ph.EP2024

Efficiently Searching for Close-in Companions around Young M Dwarfs using a Multi-year PSF Library

Aniket Sanghi, Jerry Xuan, Jason Wang +7

We present Super-RDI, a unique framework for the application of reference star differential imaging (RDI) to Keck/NIRC2 high-contrast imaging observations with the vortex coronagra…

astro-ph.EP2024★ 2 cited

Are these planets or brown dwarfs? Broadly solar compositions from high-resolution atmospheric retrievals of ~10-30 companions

Jerry W. Xuan, Chih-Chun Hsu, Luke Finnerty +32

Using Keck Planet Imager and Characterizer (KPIC) high-resolution (~35000) spectroscopy from 2.29-2.49 m, we present uniform atmospheric retrievals for eight young substellar…

astro-ph.EP2024

kappa And b is a fast rotator from KPIC High Resolution Spectroscopy

Evan C. Morris, Jason J. Wang, Chih-Chun Hsu +24

We used the Keck Planet Imager and Characterizer (KPIC) to obtain high-resolution (R35,000) K-band spectra of kappa Andromedae b, a planetary-mass companion orbiting the B9V…

astro-ph.EP2024

Friends not Foes: Strong Correlation between Inner Super-Earths and Outer Gas Giants

Marta L. Bryan, Eve J. Lee

The connection between outer gas giants and inner super-Earths reflects their formation and evolutionary histories. Past work exploring this link has suggested a tentative positive…

astro-ph.EP2024

Atmospheric Retrievals of the Young Giant Planet ROXs 42B b from Low- and High-Resolution Spectroscopy

Julie Inglis, Nicole L. Wallack, Jerry W. Xuan +7

Previous attempts have been made to characterize the atmospheres of directly imaged planets at low-resolution (R10s-100s), but the presence of clouds has often led to degener…