The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
Steven R. Majewski, Ricardo P. Schiavon, Peter M. Frinchaboy, Carlos, Allende Prieto, Robert Barkhouser, Dmitry Bizyaev, Basil Blank, Sophia, Brunner, Adam Burton, Ricardo Carrera, S. Drew Chojnowski, Katia Cunha,, Courtney Epstein, Greg Fitzgerald, Ana E. Garcia Perez

TL;DR
APOGEE, part of SDSS-III, conducted a large-scale infrared spectroscopic survey of 146,000 Milky Way stars, providing valuable data for understanding galactic structure, composition, and evolution.
Contribution
This paper details the survey's design, execution, and data products, enabling diverse astrophysical research and offering a comprehensive resource for galactic studies.
Findings
High-resolution spectra for 146,000 stars collected
Data reveals kinematic and chemical patterns across the Galaxy
Enables studies of stellar populations, interstellar medium, and star clusters
Abstract
The Apache Point Observatory Galactic Evolution Experiment (APOGEE), one of the programs in the Sloan Digital Sky Survey III (SDSS-III), has now completed its systematic, homogeneous spectroscopic survey sampling all major populations of the Milky Way. After a three year observing campaign on the Sloan 2.5-m Telescope, APOGEE has collected a half million high resolution (R~22,500), high S/N (>100), infrared (1.51-1.70 microns) spectra for 146,000 stars, with time series information via repeat visits to most of these stars. This paper describes the motivations for the survey and its overall design---hardware, field placement, target selection, operations---and gives an overview of these aspects as well as the data reduction, analysis and products. An index is also given to the complement of technical papers that describe various critical survey components in detail. Finally, we discuss…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Astronomical Observations and Instrumentation · Gamma-ray bursts and supernovae
