ABYSS. I. Targeting Strategy for the APOGEE and BOSS Young Star Survey in SDSS-V
Author
Kounkel, M.Zari, E.
Covey, K.
Tkachenko, A.
Zúñiga, C.R.
Stassun, K.
Stutz, A.M.
Stringfellow, G.
Roman-Lopes, A.
Hernández, J.
Ramírez, K.P.
Bayo, A.
Kim, J.S.
Cao, L.
Wolk, S.J.
Kollmeier, J.
López-Valdivia, R.
Rojas-Ayala, B.
Affiliation
Steward Observatory, Department of Astronomy, University of ArizonaIssue Date
2023-05-03
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American Astronomical SocietyCitation
Marina Kounkel et al 2023 ApJS 266 10Rights
© 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.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. © 2023. The Author(s). Published by the American Astronomical Society.Note
Open access journalISSN
0067-0049Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.3847/1538-4365/acc106
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Except where otherwise noted, this item's license is described as © 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.