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Alan P. Boss
Researcher at Carnegie Institution for Science
Publications - 431
Citations - 40212
Alan P. Boss is an academic researcher from Carnegie Institution for Science. The author has contributed to research in topics: Planet & Formation and evolution of the Solar System. The author has an hindex of 78, co-authored 426 publications receiving 38471 citations. Previous affiliations of Alan P. Boss include Ames Research Center & NASA Headquarters.
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Protoplanetary Disk Science Enabled by Extremely Large Telescopes
Hannah Jang-Condell,Sean D. Brittain,Alycia J. Weinberger,Michael C. Liu,Jacqueline K. Faherty,Jaehan Bae,Sean M. Andrews,Megan Ansdell,Til Birnstiel,Alan P. Boss,Laird M. Close,Thayne Currie,Steven J. Desch,Sarah Dodson-Robinson,Chuanfei Dong,Gaspard Duchêne,Catherine Espaillat,Katherine B. Follette,Eric Gaidos,Peter Gao,Nader Haghighipour,Hilairy E. Hartnett,Yasuhiro Hasegawa,Mihkel Kama,Jinyoung Serena Kim,Ágnes Kóspál,Carey M. Lisse,Wladimir Lyra,Bruce Macintosh,Dimitri Mawet,Peregrine McGehee,Michael Meyer,Eliad Peretz,Laura M. Pérez,Klaus M. Pontoppidan,Steph Sallum,Colette Salyk,Andrew Szentgyorgyi,Kevin Wagner +38 more
TL;DR: In this paper, a volume-limited survey of high-resolution spectroscopy and high-contrast imaging of the nearest protoplanetary disks that would result in an unbiased, holistic picture of planet formation as it occurs is presented.
Book ChapterDOI
Star Formation and the Solar System
TL;DR: In this article, the authors investigated the overlap between the study of other star-forming regions and the solar system and found that the overlap can be seen as a sign of the increasing ability to probe on-going star formation regions on subarc-second scales.
Journal ArticleDOI
Astrometry and radial velocities of the planet host M dwarf GJ 317: new trigonometric distance, metallicity and upper limit to the mass of GJ 317b
Guillem Anglada-Escudé,Alan P. Boss,Alycia J. Weinberger,Ian B. Thompson,R. Paul Butler,Steven S. Vogt,Eugenio J. Rivera +6 more
TL;DR: In this article, the authors obtained precision astrometry of the planet hosting M dwarf GJ 317 in the framework of the Carnegie Astrometric Planet Search project, which gave a distance determination of 15.3 pc, 65% further than previous estimates.