most citedSubstellar Objects in Nearby Young Clusters (SONYC): The bottom of the Initial Mass Function in NGC1333

73 citations · 97 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2026

An early look at how gas giants shape small planet bulk compositions

Joseph Y. Tang, Marta L. Bryan, Eve J. Lee

Gas giants may shape the reservoir of solids and gas in the inner disk in which the small planets assemble. To test this possibility, we collect a sample of 43 exoplanetary systems…

astro-ph.EP2026★ 12 cited

The compositions of the HR 8799 planets reflect accretion of both solids and metal-enriched gas

Jerry W. Xuan, Jean-Baptiste Ruffio, Yayaati Chachan +24

With four giant planets (, $T_\rm{eff}\sim900-1200$ K) orbiting between 15-70 au, HR 8799 provides an unparalleled testbed for studying giant planet formatio…

astro-ph.EP2026

Planet-Planet Scattering Explains the Mass-Eccentricity Relation of Warm Jupiters

Jiayin Dong, Eve J. Lee, Eiichiro Kokubo +2

Warm giant planets with orbital periods of tens of days exhibit a positive correlation between mass and eccentricity. We interpret this trend as the outcome of planet-planet scatte…

astro-ph.EP2026★ 12 cited

Jupiter-like uniform metal enrichment in a system of multiple giant exoplanets

Jean-Baptiste Ruffio, Jerry W. Xuan, Yayaati Chachan +15

The accretion of icy and rocky solids during the formation of a gas giant planet is poorly constrained and challenging to model. Refractory species, like sulfur, are only present i…

astro-ph.SR2009★ 73 cited

Substellar Objects in Nearby Young Clusters (SONYC): The bottom of the Initial Mass Function in NGC1333

Alexander Scholz, Vincent Geers, Ray Jayawardhana +4

SONYC -- Substellar Objects in Nearby Young Clusters -- is a survey program to investigate the frequency and properties of substellar objects with masses down to a few times that o…