Publication Title
Astrophysical Journal, Supplement Series
Document Type
Article
Department or Program
Physics and Astronomy
Publication Date
6-2020
Abstract
This paper documents the 16th data release (DR16) from the Sloan Digital Sky Surveys (SDSS), the fourth and penultimate from the fourth phase (SDSS-IV). This is the first release of data from the Southern Hemisphere survey of the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2); new data from APOGEE-2 North are also included. DR16 is also notable as the final data release for the main cosmological program of the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), and all raw and reduced spectra from that project are released here. DR16 also includes all the data from the Time Domain Spectroscopic Survey and new data from the SPectroscopic IDentification of ERosita Survey programs, both of which were co-observed on eBOSS plates. DR16 has no new data from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey (or the MaNGA Stellar Library "MaStar"). We also preview future SDSS-V operations (due to start in 2020), and summarize plans for the final SDSS-IV data release (DR17).
Recommended Citation
Avila-Reese, V., Badenes, C., Bautista, J., Beers, T. C., Bershady, M., Bird, J., Bizyaev, D., Borissova, J., Bovy, J., Brinkmann, J., Brownstein, J. R., Bundy, K., Burgasser, A., Capasso, R., Chabanier, S., Chaplin, W., Cherinka, B., Chiappini, C., Doohyun Choi, P., … Davies, R. (2020). The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra. The Astrophysical Journal. Supplement Series, 249(1), 3–.
Copyright Note
© 2020. 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/ab929e