Abstract
We describe the Sloan Digital Sky Survey IV (SDSS-IV), a project encompassing three major spectroscopic programs. The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is observing hundreds of thousands of Milky Way stars at high resolution and high signal-to-noise ratios in the near-infrared. The Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey is obtaining spatially resolved spectroscopy for thousands of nearby galaxies (median z ∼ 0.03). The extended Baryon Oscillation Spectroscopic Survey (eBOSS) is mapping the galaxy, quasar, and neutral gas distributions between z ~ 0.6 and 3.5 to constrain cosmology using baryon acoustic oscillations, redshift space distortions, and the shape of the power spectrum. Within eBOSS, we are conducting two major subprograms: the SPectroscopic IDentification of eROSITA Sources (SPIDERS), investigating X-ray AGNs and galaxies in X-ray clusters, and the Time Domain Spectroscopic Survey (TDSS), obtaining spectra of variable sources. All programs use the 2.5 m Sloan Foundation Telescope at the Apache Point Observatory; observations there began in Summer 2014. APOGEE-2 also operates a second near-infrared spectrograph at the 2.5 m du Pont Telescope at Las Campanas Observatory, with observations beginning in early 2017. Observations at both facilities are scheduled to continue through 2020. In keeping with previous SDSS policy, SDSS-IV provides regularly scheduled public data releases; the first one, Data Release 13, was made available in 2016 July.
| Original language | English |
|---|---|
| Article number | 28 |
| Journal | Astronomical Journal |
| Volume | 154 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 1 Jul 2017 |
Keywords
- cosmology: observations
- galaxies: general
- Galaxy: general
- instrumentation: spectrographs
- stars: general
- surveys
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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In: Astronomical Journal, Vol. 154, No. 1, 28, 01.07.2017.
Research output: Contribution to journal › Review article › peer-review
TY - JOUR
T1 - Sloan Digital Sky Survey IV
T2 - Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
AU - Blanton, Michael R.
AU - Bershady, Matthew A.
AU - Abolfathi, Bela
AU - Albareti, Franco D.
AU - Prieto, Carlos Allende
AU - Almeida, Andres
AU - Alonso-García, Javier
AU - Anders, Friedrich
AU - Anderson, Scott F.
AU - Andrews, Brett
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AU - Aragón-Salamanca, Alfonso
AU - Argudo-Fernández, Maria
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AU - Aubourg, Eric
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AU - Bartosz, Curtis
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AU - Burtin, Etienne
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AU - Carigi, Maria Leticia Delgado
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AU - Cherinka, Brian
AU - Cheung, Edmond
AU - Chew, Yilen Gómez Maqueo
AU - Chiappini, Cristina
AU - Choi, Peter Doohyun
AU - Chojnowski, Drew
AU - Chuang, Chia Hsun
AU - Chung, Haeun
AU - Cirolini, Rafael Fernando
AU - Clerc, Nicolas
AU - Cohen, Roger E.
AU - Comparat, Johan
AU - Costa, Luiz Da
AU - Cousinou, Marie Claude
AU - Covey, Kevin
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AU - Lee, Nathan De
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AU - Mille, Francesco Di
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AU - Stringfellow, Guy S.
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AU - Zhu, Guangtun B.
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N1 - Publisher Copyright: © 2017. The American Astronomical Society. All rights reserved.
PY - 2017/7/1
Y1 - 2017/7/1
N2 - We describe the Sloan Digital Sky Survey IV (SDSS-IV), a project encompassing three major spectroscopic programs. The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is observing hundreds of thousands of Milky Way stars at high resolution and high signal-to-noise ratios in the near-infrared. The Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey is obtaining spatially resolved spectroscopy for thousands of nearby galaxies (median z ∼ 0.03). The extended Baryon Oscillation Spectroscopic Survey (eBOSS) is mapping the galaxy, quasar, and neutral gas distributions between z ~ 0.6 and 3.5 to constrain cosmology using baryon acoustic oscillations, redshift space distortions, and the shape of the power spectrum. Within eBOSS, we are conducting two major subprograms: the SPectroscopic IDentification of eROSITA Sources (SPIDERS), investigating X-ray AGNs and galaxies in X-ray clusters, and the Time Domain Spectroscopic Survey (TDSS), obtaining spectra of variable sources. All programs use the 2.5 m Sloan Foundation Telescope at the Apache Point Observatory; observations there began in Summer 2014. APOGEE-2 also operates a second near-infrared spectrograph at the 2.5 m du Pont Telescope at Las Campanas Observatory, with observations beginning in early 2017. Observations at both facilities are scheduled to continue through 2020. In keeping with previous SDSS policy, SDSS-IV provides regularly scheduled public data releases; the first one, Data Release 13, was made available in 2016 July.
AB - We describe the Sloan Digital Sky Survey IV (SDSS-IV), a project encompassing three major spectroscopic programs. The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is observing hundreds of thousands of Milky Way stars at high resolution and high signal-to-noise ratios in the near-infrared. The Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey is obtaining spatially resolved spectroscopy for thousands of nearby galaxies (median z ∼ 0.03). The extended Baryon Oscillation Spectroscopic Survey (eBOSS) is mapping the galaxy, quasar, and neutral gas distributions between z ~ 0.6 and 3.5 to constrain cosmology using baryon acoustic oscillations, redshift space distortions, and the shape of the power spectrum. Within eBOSS, we are conducting two major subprograms: the SPectroscopic IDentification of eROSITA Sources (SPIDERS), investigating X-ray AGNs and galaxies in X-ray clusters, and the Time Domain Spectroscopic Survey (TDSS), obtaining spectra of variable sources. All programs use the 2.5 m Sloan Foundation Telescope at the Apache Point Observatory; observations there began in Summer 2014. APOGEE-2 also operates a second near-infrared spectrograph at the 2.5 m du Pont Telescope at Las Campanas Observatory, with observations beginning in early 2017. Observations at both facilities are scheduled to continue through 2020. In keeping with previous SDSS policy, SDSS-IV provides regularly scheduled public data releases; the first one, Data Release 13, was made available in 2016 July.
KW - cosmology: observations
KW - galaxies: general
KW - Galaxy: general
KW - instrumentation: spectrographs
KW - stars: general
KW - surveys
UR - http://www.scopus.com/inward/record.url?scp=85024504231&partnerID=8YFLogxK
U2 - 10.3847/1538-3881/aa7567
DO - 10.3847/1538-3881/aa7567
M3 - Review article
AN - SCOPUS:85024504231
SN - 0004-6256
VL - 154
JO - Astronomical Journal
JF - Astronomical Journal
IS - 1
M1 - 28
ER -