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The completed SDSS-IV extended baryon oscillation spectroscopic survey: growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the emission-line galaxy sample
- Source :
- Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 499 (4), pp.5527-5546. ⟨10.1093/mnras/staa3050⟩, Monthly Notices of the Royal Astronomical Society, 2020, 499 (4), pp.5527-5546. ⟨10.1093/mnras/staa3050⟩
- Publisher :
- OXFORD UNIV PRESS
-
Abstract
- We present the anisotropic clustering of emission line galaxies (ELGs) from the Sloan Digital Sky Survey IV (SDSS-IV) extended Baryon Oscillation Spectroscopic Survey (eBOSS) Data Release 16 (DR16). Our sample is composed of 173,736 ELGs covering an area of 1170 deg$^2$ over the redshift range $0.6 \leq z \leq 1.1$. We use the Convolution Lagrangian Perturbation Theory in addition to the Gaussian Streaming Redshift-Space Distortions to model the Legendre multipoles of the anisotropic correlation function. We show that the eBOSS ELG correlation function measurement is affected by the contribution of a radial integral constraint that needs to be modelled to avoid biased results. To mitigate the effect from unknown angular systematics, we adopt a modified correlation function estimator that cancels out the angular modes from the clustering. At the effective redshift, $z_{\rm eff}=0.85$, including statistical and systematical uncertainties, we measure the linear growth rate of structure $f\sigma_8(z_{\rm eff}) = 0.35\pm0.10$, the Hubble distance $D_H(z_{\rm eff})/r_{\rm drag} = 19.1^{+1.9}_{-2.1}$ and the comoving angular diameter distance $D_M(z_{\rm eff})/r_{\rm drag} = 19.9\pm1.0$. These results are in agreement with the Fourier space analysis, leading to consensus values of: $f\sigma_8(z_{\rm eff}) = 0.315\pm0.095$, $D_H(z_{\rm eff})/r_{\rm drag} = 19.6^{+2.2}_{-2.1}$ and $D_M(z_{\rm eff})/r_{\rm drag} = 19.5\pm1.0$, consistent with $\Lambda$CDM model predictions with Planck parameters.<br />Comment: A summary of all SDSS BAO and RSD measurements with accompanying legacy figures can be found here: https://www.sdss.org/science/final-bao-and-rsd-measurements/ . The full cosmological interpretation of these measurements can be found here: https://www.sdss.org/science/cosmology-results-from-eboss/
- Subjects :
- Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Galaxies distances and redshift
reconstruction
[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
FOS: Physical sciences
Large scale structure of Universe
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Correlation function (quantum field theory)
distance scale
01 natural sciences
large-scale structure
efficient
0103 physical sciences
evolution
quasar sample
Emission spectrum
Perturbation theory
dark energy
010303 astronomy & astrophysics
Legendre polynomials
power-spectrum analysis
Physics
large-scale structure of universe
model
010308 nuclear & particles physics
Angular diameter distance
Astronomy and Astrophysics
Cosmology observations
acoustic-oscillations
Galaxy
Redshift
Baryon
Space and Planetary Science
cosmology: observations
digital sky survey
galaxies: distances and redshifts
cosmology
Astrophysics - Cosmology and Nongalactic Astrophysics
Subjects
Details
- ISSN :
- 00358711 and 13652966
- Database :
- OpenAIRE
- Journal :
- Monthly Notices of the Royal Astronomical Society, Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 499 (4), pp.5527-5546. ⟨10.1093/mnras/staa3050⟩, Monthly Notices of the Royal Astronomical Society, 2020, 499 (4), pp.5527-5546. ⟨10.1093/mnras/staa3050⟩
- Accession number :
- edsair.doi.dedup.....4247d935c467eee5fdce457daaddf5ec
- Full Text :
- https://doi.org/10.1093/mnras/staa3050⟩