Publication Title
Astrophysical Journal, Supplement Series
Document Type
Article
Department or Program
Physics and Astronomy
Publication Date
3-2022
Abstract
This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the complete release of the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, which reached its goal of surveying over 10,000 nearby galaxies. The complete release of the MaNGA Stellar Library accompanies this data, providing observations of almost 30,000 stars through the MaNGA instrument during bright time. DR17 also contains the complete release of the Apache Point Observatory Galactic Evolution Experiment 2 survey that publicly releases infrared spectra of over 650,000 stars. The main sample from the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), as well as the subsurvey Time Domain Spectroscopic Survey data were fully released in DR16. New single-fiber optical spectroscopy released in DR17 is from the SPectroscipic IDentification of ERosita Survey subsurvey and the eBOSS-RM program. Along with the primary data sets, DR17 includes 25 new or updated value-added catalogs. This paper concludes the release of SDSS-IV survey data. SDSS continues into its fifth phase with observations already underway for the Milky Way Mapper, Local Volume Mapper, and Black Hole Mapper surveys.
Recommended Citation
Filiz Ak, N., Andrews, B. H., Anguiano, B., Aquino-Ortíz, E., Argudo-Fernández, M., Ata, M., Aubert, M., Barger, K., Beers, T. C., Bernardi, M., Bidin, C. M., Bird, J. C., Bizyaev, D., Blanc, G. A., Blanton, M. R., Borissova, J., Buchner, J., Bundy, K., Bureau, M., … Cherinka, B. (2022). The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. The Astrophysical Journal, 259(2), 35–.
Copyright Note
© 2022. The Authors. Published by the American Astronomical Society.
Required Publisher's Statement
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
Comments
Original version is available from the publisher at: https://doi.org/10.3847/1538-4365/ac4414