Kounkel, Marina, Zari, Eleonora, Covey, Kevin, Tkachenko, Andrew, Zuniga, Carlos Roman, Stassun, Keivan, Stutz, Amelia M., Stringfellow, Guy, Roman-Lopes, Alexandre, Hernandez, Jesus, Ramirez, Karla Pena, Bayo, Amelia, Kim, Jinyoung Serena, Cao, Lyra, Wolk, Scott J., Kollmeier, Juna, Lopez-Valdivia, Ricardo, Rojas-Ayala, Barbara2024-11-272024-11-272023/05/010067-0049http://dx.doi.org/10.3847/1538-4365/acc106https://publicacionesabiertas.userena.cl/handle/123456789/119The fifth iteration of the Sloan Digital Sky Survey is set to obtain optical and near-infrared spectra of similar to 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 similar to 10(5) 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 similar to 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.MAIN-SEQUENCE STARS, DIGITAL SKY SURVEY, GAIA-ESO SURVEY, LOW-MASS STARS, STELLAR OBJECTS, VELOCITY DISPERSION, LAMBDA ORIONIS, FORMING REGION, GALACTIC PLANE, CLASSIFICATIONArticle