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20172025
most citedDetection and Bulk Properties of the HR 8799 Planets with High Resolution Spectroscopy

79 citations · 370 across the 12 of their papers we have counts for

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astro-ph.EP20211 cited

Obliquity Constraints on the Planetary-mass Companion HD 106906 b

Marta L. Bryan, Eugene Chiang, Caroline V. Morley +2

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-ma…

astro-ph.EP202179 cited

Detection and Bulk Properties of the HR 8799 Planets with High Resolution Spectroscopy

Jason J. Wang, Jean-Baptiste Ruffio, Evan Morris +49

Using the Keck Planet Imager and Characterizer (KPIC), we obtained high-resolution (R35,000) -band spectra of the four planets orbiting HR 8799. We clearly detected \water…

astro-ph.EP2020

As the Worlds Turn: Constraining Spin Evolution in the Planetary-Mass Regime

Marta L. Bryan, Sivan Ginzburg, Eugene Chiang +4

To understand how planetary spin evolves and traces planet formation processes, we measure rotational line broadening in eight planetary-mass objects (PMOs) of various ages (1--800…

astro-ph.EP202055 cited

Strong Near-Infrared Spectral Variability of the Young Cloudy L Dwarf Companion VHS J1256-1257 b

Brendan P. Bowler, Yifan Zhou, Caroline V. Morley +4

Rotationally-modulated variability of brown dwarfs and giant planets provides unique information about their surface brightness inhomogeneities, atmospheric circulation, cloud evol…

astro-ph.EP2020

Obliquity Constraints on an Extrasolar Planetary-Mass Companion

Marta L. Bryan, Eugene Chiang, Brendan P. Bowler +8

We place the first constraints on the obliquity of a planetary-mass companion (PMC) outside of the Solar System. Our target is the directly imaged system 2MASS J01225093-2439505 (2…

astro-ph.EP202023 cited

A Rotation Rate for the Planetary-Mass Companion DH Tau b

Jerry W. Xuan, Marta L. Bryan, Heather A. Knutson +3

DH Tau b is a young planetary-mass companion orbiting at a projected separation of 320 AU from its 2 Myr old host star DH Tau. With an estimated mass of