activity
20012023
most citedKepler Mission Design, Realized Photometric Performance, and Early Science

1.2k citations · 11.4k across the 102 of their papers we have counts for

collaborators

102 papers

astro-ph.EP2023

Forming Gas Giants Around a Range of Protostellar M-dwarfs by Gas Disk Gravitational Instability

Alan P. Boss, Shubham Kanodia

Recent discoveries of gas giant exoplanets around M-dwarfs (GEMS) from transiting and radial velocity (RV) surveys are difficult to explain with core-accretion models. We present h…

astro-ph.IM2023

Enabling Exoplanet Demographics Studies with Standardized Exoplanet Survey Meta-Data

Prepared by the ExoPAG Science Interest Group, 2 on Exoplanet Demographics, Jessie L. Christiansen +18

Goal 1 of the National Academies of Science, Engineering and Mathematics Exoplanet Science Strategy is "to understand the formation and evolution of planetary systems as products o…

astro-ph.EP2022★ 11 cited

Orbital Migration of Protoplanets in a Marginally Gravitationally Unstable Disk. II. Migration, Merging, and Ejection

Alan P. Boss

Protoplanets formed in a marginally gravitationally unstable (MGU) disk by either core accretion or disk instability will be subject to dynamical interactions with massive spiral a…

astro-ph.EP2022★ 50 cited

TOI-5205 b: A Short-period Jovian Planet Transiting a Mid-M Dwarf

Shubham Kanodia, Suvrath Mahadevan, Jessica Libby-Roberts +27

We present the discovery of TOI-5205~b, a transiting Jovian planet orbiting a solar metallicity M4V star, which was discovered using Transiting Exoplanet Survey Satellite photometr…

astro-ph.EP2022★ 3 cited

Possible Implications of Relatively High Levels of Initial Fe in Iron Meteorites for the Non-Carbonaceous -- Carbonaceous Meteorite Dichotomy and Solar Nebula Formation

Alan P. Boss

Cook et al. (2021) found that iron meteorites have an initial abundance ratio of the short-lived isotope Fe to the stable isotope Fe of Fe/Fe $(6…

astro-ph.EP2021★ 9 cited

Flux-Limited Diffusion Approximation Models of Giant Planet Formation by Disk Instability. II. Quadrupled Spatial Resolution

Alan P. Boss

While collisional accumulation is nearly universally accepted as the formation mechanism of rock and ice worlds, the situation regarding gas giant planet formation is more nuanced.…