ABYSS. I. Targeting Strategy for the APOGEE and BOSS Young Star Survey in SDSS-V

Author:

Kounkel MarinaORCID,Zari EleonoraORCID,Covey KevinORCID,Tkachenko AndrewORCID,Zúñiga Carlos RománORCID,Stassun KeivanORCID,Stutz Amelia M.ORCID,Stringfellow GuyORCID,Roman-Lopes AlexandreORCID,Hernández JesúsORCID,Ramírez Karla PeñaORCID,Bayo AmeliaORCID,Kim Jinyoung SerenaORCID,Cao LyraORCID,Wolk Scott J.ORCID,Kollmeier JunaORCID,López-Valdivia RicardoORCID,Rojas-Ayala BárbaraORCID

Abstract

Abstract The fifth iteration of the Sloan Digital Sky Survey is set to obtain optical and near-infrared spectra of ∼5 million stars of all ages and masses throughout the Milky Way. As a part of these efforts, APOGEE and BOSS Young Star Survey (ABYSS) will observe ∼105 stars with ages <30 Myr that have been selected using a set of homogeneous selection functions that make use of different tracers of youth. The ABYSS targeting strategy we describe in this paper is aimed to provide the largest spectroscopic census of young stars to date. It consists of eight different types of selection criteria that take the position on the H-R diagram, infrared excess, variability, as well as the position in phase space in consideration. The resulting catalog of ∼200,000 sources (of which a half are expected to be observed) provides representative coverage of the young Galaxy, including both nearby diffuse associations as well as more distant massive complexes, reaching toward the inner Galaxy and the Galactic center.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

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