The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and early data
Abstract
All rights reserved. In a six-year program started in 2014 July, the Extended Baryon Oscillation Spectroscopic Survey (eBOSS) will conduct novel cosmological observations using the BOSS spectrograph at Apache Point Observatory. These observations will be conducted simultaneously with the Time Domain Spectroscopic Survey (TDSS) designed for variability studies and the Spectroscopic Identification of eROSITA Sources (SPIDERS) program designed for studies of X-ray sources. In particular, eBOSS will measure with percent-level precision the distance-redshift relation with baryon acoustic oscillations (BAO) in the clustering of matter. eBOSS will use four different tracers of the underlying matter density field to vastly expand the volume covered by BOSS and map the large-scale-structures over the relatively unconstrained redshift range 0.6 < z < 2.2. Using more than 250,000 new, spectroscopically confirmed luminous red galaxies at a median redshift z = 0.72, we project that eBOSS will yield measurements of the angular diameter distance d A (z) to an accuracy of 1.2% and measurements of H(z) to 2.1% when combined with the z > 0.6 sample of BOSS galaxies. With ~195,000 new emission line galaxy redshifts, we expect BAO measurements of d A (z) to an accuracy of 3.1% and H(z) to 4.7% at an effectivemore »
- Authors:
-
- Univ. of Utah, Salt Lake City, UT (United States). et al.
- Publication Date:
- Research Org.:
- Brookhaven National Laboratory (BNL), Upton, NY (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1252211
- Alternate Identifier(s):
- OSTI ID: 1247979; OSTI ID: 1379071
- Report Number(s):
- arXiv:1508.04473; FERMILAB-PUB-15-643-AE; BNL-112053-2016-JA
Journal ID: ISSN 1538-3881; 1388477
- Grant/Contract Number:
- AC02-07CH11359; SC0012704; AC02-05CH11231
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astronomical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astronomical Journal (Online); Journal Volume: 151; Journal Issue: 2; Journal ID: ISSN 1538-3881
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; cosmology: observations
Citation Formats
Dawson, Kyle S. The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and early data. United States: N. p., 2016.
Web. doi:10.3847/0004-6256/151/2/44.
Dawson, Kyle S. The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and early data. United States. https://doi.org/10.3847/0004-6256/151/2/44
Dawson, Kyle S. Thu .
"The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and early data". United States. https://doi.org/10.3847/0004-6256/151/2/44. https://www.osti.gov/servlets/purl/1252211.
@article{osti_1252211,
title = {The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and early data},
author = {Dawson, Kyle S.},
abstractNote = {All rights reserved. In a six-year program started in 2014 July, the Extended Baryon Oscillation Spectroscopic Survey (eBOSS) will conduct novel cosmological observations using the BOSS spectrograph at Apache Point Observatory. These observations will be conducted simultaneously with the Time Domain Spectroscopic Survey (TDSS) designed for variability studies and the Spectroscopic Identification of eROSITA Sources (SPIDERS) program designed for studies of X-ray sources. In particular, eBOSS will measure with percent-level precision the distance-redshift relation with baryon acoustic oscillations (BAO) in the clustering of matter. eBOSS will use four different tracers of the underlying matter density field to vastly expand the volume covered by BOSS and map the large-scale-structures over the relatively unconstrained redshift range 0.6 < z < 2.2. Using more than 250,000 new, spectroscopically confirmed luminous red galaxies at a median redshift z = 0.72, we project that eBOSS will yield measurements of the angular diameter distance d A (z) to an accuracy of 1.2% and measurements of H(z) to 2.1% when combined with the z > 0.6 sample of BOSS galaxies. With ~195,000 new emission line galaxy redshifts, we expect BAO measurements of d A (z) to an accuracy of 3.1% and H(z) to 4.7% at an effective redshift of z = 0.87. A sample of more than 500,000 spectroscopically confirmed quasars will provide the first BAO distance measurements over the redshift range 0.9 < z < 2.2, with expected precision of 2.8% and 4.2% on d A (z) and H(z), respectively. Finally, with 60,000 new quasars and re-observation of 60,000 BOSS quasars, we will obtain new Lyα forest measurements at redshifts z > 2.1; these new data will enhance the precision of d A (z) and H(z) at z > 2.1 by a factor of 1.44 relative to BOSS. Furthermore, eBOSS will provide improved tests of General Relativity on cosmological scales through redshift-space distortion measurements, improved tests for non-Gaussianity in the primordial density field, and new constraints on the summed mass of all neutrino species. Here, we provide an overview of the cosmological goals, spectroscopic target sample, demonstration of spectral quality from early data, and projected cosmological constraints from eBOSS.},
doi = {10.3847/0004-6256/151/2/44},
journal = {The Astronomical Journal (Online)},
number = 2,
volume = 151,
place = {United States},
year = {Thu Feb 04 00:00:00 EST 2016},
month = {Thu Feb 04 00:00:00 EST 2016}
}
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New parametrized equation of state for dark energy surveys
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Constraining power of cosmological observables: Blind redshift spots and optimal ranges
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Dark Energy Survey Year 1 results: Measurement of the baryon acoustic oscillation scale in the distribution of galaxies to redshift 1
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Deep CFHT Y -band Imaging of VVDS-F22 Field. II. Quasar Selection and Quasar Luminosity Function
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The Circumgalactic Medium of eBOSS Emission Line Galaxies: Signatures of Galactic Outflows in Gas Distribution and Kinematics
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Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
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Cross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic and Photometric Galaxy Surveys
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SDSS-IV MaStar: A Large and Comprehensive Empirical Stellar Spectral Library—First Release
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The Second Data Release of the Beijing–Arizona Sky Survey
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The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA-derived Quantities, Data Visualization Tools, and Stellar Library
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Learning to predict the cosmological structure formation
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Cosmology with intensity mapping techniques using atomic and molecular lines
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Dark Energy Survey Year 1 results: measurement of the baryon acoustic oscillation scale in the distribution of galaxies to redshift 1
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Dark energy, α-attractors, and large-scale structure surveys
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Searching for light relics with large-scale structure
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The first 62 AGN observed with SDSS-IV MaNGA – II. Resolvedstellar populations
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Dark Energy Survey Year 1 Results: A Precise H0 Estimate from DES Y1, BAO, and D/H Data
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The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration space
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Results of a systematic search for outburst events in 1.4 million galaxies
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The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2
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J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions
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The effect of assembly bias on redshift-space distortions
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Reducing the two-loop large-scale structure power spectrum to low-dimensional, radial integrals
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Imprints of primordial non-Gaussianity on gravitational wave spectrum
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Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
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The Sloan Digital Sky Survey Quasar Catalog: twelfth data release
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The Sdss-Iv Extended Baryon Oscillation Spectroscopic Survey: Luminous red Galaxy Target Selection
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An Evaluation of Cosmological Models from the Expansion and Growth of Structure Measurements
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Galaxies Probing Galaxies in PRIMUS. II. The Coherence Scale of the Cool Circumgalactic Medium
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Spectacular Hubble Space Telescope Observations of the Coma Galaxy D100 and Star Formation in Its Ram Pressure–stripped Tail
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The Extremely Luminous Quasar Survey in the Sloan Digital Sky Survey Footprint. III. The South Galactic Cap Sample and the Quasar Luminosity Function at Cosmic Noon
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The Time-domain Spectroscopic Survey: Radial Velocity Variability in Dwarf Carbon Stars
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The Extended Baryon Oscillation Spectroscopic Survey: Measuring the Cross-correlation between the Mg ii Flux Transmission Field and Quasars and Galaxies at z = 0.59
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Classification of Broad Absorption Line Quasars with a Convolutional Neural Network
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Principal shapes and squeezed limits in the effective field theory of large scale structure
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Measuring the scale of cosmic homogeneity with SDSS-IV DR14 quasars
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On the limitations of statistical absorption studies with the Sloan Digital Sky Surveys I–III
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Exploring relations between BCG and cluster properties in the SPectroscopic IDentification of eROSITA Sources survey from 0.05
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Linear density perturbations in multifield coupled quintessence
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EFT of large scale structures in redshift space
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Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
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The SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations at Redshift of 0.72 with the DR14 Luminous Red Galaxy Sample
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The Extremely Luminous Quasar Survey in the Sloan Digital Sky Survey Footprint. II. The North Galactic Cap Sample
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Active galactic nuclei and their large-scale structure: an eROSITA mock catalogue
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Observable predictions for massive-neutrino cosmologies with model-independent dark energy
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Cosmology with intensity mapping techniques using atomic and molecular lines
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Linear Density Perturbations in Multifield Coupled Quintessence
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- arXiv
The Sloan Digital Sky Survey Quasar Catalog: twelfth data release
text, January 2016
- Pâris, Isabelle; Petitjean, Patrick; Ross, Nicholas P.
- arXiv
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: theoretical systematics and Baryon Acoustic Oscillations in the galaxy correlation function
text, January 2016
- Vargas-Magaña, Mariana; Ho, Shirley; Cuesta, Antonio J.
- arXiv
Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
text, January 2017
- Blanton, Michael R.; Bershady, Matthew A.; Abolfathi, Bela
- arXiv
Effect of Massive Neutrinos on the Position of Cold Dark Matter Halo: Revealed via Delaunay Triangulation Void
text, January 2017
- Qin, Jian; Liang, Yu; Zhao, Cheng
- arXiv
The Sloan Digital Sky Survey Quasar Catalog: Fourteenth Data Release
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- Pâris, I.; Petitjean, P.; Aubourg, E.
- arXiv
The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations at redshift of 0.72 with the DR14 Luminous Red Galaxy Sample
text, January 2017
- Bautista, Julian E.; Vargas-Magaña, Mariana; Dawson, Kyle S.
- arXiv
Deep CFHT Y-band Imaging of VVDS-F22 Field: II. Quasar Selection and Quasar Luminosity Function
text, January 2018
- Yang, Jinyi; Wu, Xue-Bing; Liu, Dezi
- arXiv
The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the evolution of the growth rate using redshift space distortions between redshift 0.8 and 2.2
text, January 2018
- Ruggeri, Rossana; Percival, Will J.; Marin, Hector Gil
- arXiv
The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights
text, January 2018
- Zhao, Gong-Bo; Wang, Yuting; Saito, Shun
- arXiv
The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2
text, January 2018
- Zarrouk, Pauline; Burtin, Etienne; Gil-Marin, Hector
- arXiv
The Aemulus Project III: Emulation of the Galaxy Correlation Function
text, January 2018
- Zhai, Zhongxu; Tinker, Jeremy L.; Becker, Matthew R.
- arXiv
Overview of the DESI Legacy Imaging Surveys
text, January 2018
- Dey, Arjun; Schlegel, David J.; Lang, Dustin
- arXiv
The VIMOS Public Extragalactic Redshift Survey (VIPERS): Unbiased clustering estimate with VIPERS slit assignment
text, January 2018
- Mohammad, F. G.; Bianchi, D.; Percival, W. J.
- arXiv
Constraining Sub-Parsec Binary Supermassive Black Holes in Quasars with Multi-Epoch Spectroscopy. III. Candidates from Continued Radial Velocity Tests
text, January 2018
- Guo, Hengxiao; Liu, Xin; Shen, Yue
- arXiv
Imprints of Primordial Non-Gaussianity on Gravitational Wave Spectrum
text, January 2018
- Unal, Caner
- arXiv
J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions
text, January 2019
- Costa, A. A.; Marcondes, R. J. F.; Landim, R. G.
- arXiv
Representation learning for automated spectroscopic redshift estimation
text, January 2019
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- arXiv
The correlations between optical/UV broad lines and X-ray emission for a large sample of quasars
text, January 2019
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- arXiv