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Mapping the Distant and Metal-poor Milky Way with SDSS-V

The fifth-generation Sloan Digital Sky Survey (SDSS-V) is conducting the first all-sky low-resolution spectroscopic survey of the Milky Way’s (MW) stellar halo. We describe the stellar parameter pipeline for the SDSS-V halo survey, which simultaneously models spectra, broadband photometry, and paral...

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Hoofdauteurs: Vedant Chandra, Phillip A. Cargile, Alexander P. Ji, Charlie Conroy, Hans-Walter Rix, Emily Cunningham, Bruno Dias, Chervin Laporte, William Cerny, Guilherme Limberg, Avrajit Bandyopadhyay, Ana Bonaca, Andrew R. Casey, John Donor, José G. Fernández-Trincado, Peter M. Frinchaboy, Pramod Gupta, Keith Hawkins, Jennifer A. Johnson, Juna A. Kollmeier, Madeline Lucey, Ilija Medan, Szabolcs Mészáros, Sean Morrison, José Sánchez-Gallego, Andrew K. Saydjari, Conor Sayres, Kevin C. Schlaufman, Keivan G. Stassun, Jamie Tayar, Zachary Way
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: IOP Publishing 2026-01-01
Reeks:The Astrophysical Journal
Onderwerpen:
Halo stars
Milky Way stellar halo
Spectroscopy
Stellar properties
Stellar abundances
Stellar distance
Online toegang:https://doi.org/10.3847/1538-4357/ae448a
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