KiDS+2dFLenS+GAMA

Autor: C. D. Leonard, Shahab Joudaki, Christian Wolf, Karl Glazebrook, Edwin A. Valentijn, Henk Hoekstra, C. Lidman, Konrad Kuijken, Maciej Bilicki, Marika Asgari, Thomas Erben, Chris Blake, Benjamin Joachimi, Jon Loveday, David Parkinson, Catherine Heymans, Joachim Harnois-Déraps, A. Choi, Alexandra Amon, Hendrik Hildebrandt
Přispěvatelé: Astronomy
Jazyk: angličtina
Rok vydání: 2018
Předmět:
observations [Surveys
cosmology]

Cosmology and Nongalactic Astrophysics (astro-ph.CO)
LENSING SURVEY
General relativity
COSMIC SHEAR
PARAMETER CONSTRAINTS
media_common.quotation_subject
Cosmic microwave background
FOS: Physical sciences
Large-scale structure of universe
Astrophysics
01 natural sciences
Cosmology
gravitational lensing: weak
surveys
0103 physical sciences
LARGE-SCALE STRUCTURE
GENERAL-RELATIVITY
010303 astronomy & astrophysics
QC
Weak gravitational lensing
Statistic
QB
media_common
Physics
surveys
cosmology: observations
large-scale structure of Universe

010308 nuclear & particles physics
Astronomy and Astrophysics
Galaxy
Universe
Amplitude
Space and Planetary Science
cosmology: observations
COVARIANCE MATRICES
large-scale structure of Universe
SURVEY DESIGN
WEAK
weak [Gravitational lensing]
REDSHIFT-SPACE
Astrophysics - Cosmology and Nongalactic Astrophysics
GAMA GALAXY GROUPS
Zdroj: Monthly Notices of the Royal Astronomical Society, 479(3), 3422-3437. Oxford University Press
Amon, A, Blake, C, Heymans, C, Leonard, C D, Asgari, M, Bilicki, M, Choi, A, Erben, T, Glazebrook, K, Harnois-Déraps, J, Hildebrandt, H, Hoekstra, H, Joachimi, B, Joudaki, S, Kuijken, K, Lidman, C, Loveday, J, Parkinson, D, Valentijn, E A & Wolf, C 2018, ' KiDS+2dFLenS+GAMA : Testing the cosmological model with the E G statistic ', Monthly Notices of the Royal Astronomical Society, vol. 479, no. 3, pp. 3422-3437 . https://doi.org/10.1093/mnras/sty1624
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 479(3), 3422-3437
ISSN: 1365-2966
0035-8711
DOI: 10.1093/mnras/sty1624
Popis: We present a new measurement of $E_{\rm G}$, which combines measurements of weak gravitational lensing, real-space galaxy clustering and redshift space distortions. This statistic was proposed as a consistency test of General Relativity (GR) that is insensitive to linear, deterministic galaxy bias and the matter clustering amplitude. We combine deep imaging data from KiDS with overlapping spectroscopy from 2dFLenS, BOSS DR12 and GAMA and find $E_{\rm G}(\overline{z}=0.267)=0.43 \pm 0.13$ (GAMA), $E_{\rm G}(\overline{z}=0.305)=0.27 \pm 0.08$ (LOWZ+2dFLOZ) and $E_{\rm G}(\overline{z}=0.554)=0.26 \pm 0.07$ (CMASS+2dFHIZ). We demonstrate that the existing tension in the value of the matter density parameter hinders the robustness of this statistic as solely a test of GR. We find that our $E_{\rm G}$ measurements, as well as existing ones in the literature, favour a lower matter density cosmology than the Cosmic Microwave Background. For a flat $\Lambda$CDM Universe and assuming GR, we find $\Omega_{\rm m}(z=0)=0.25\pm0.03$. With this paper we publicly release the 2dFLenS dataset at: \url{http://2dflens.swin.edu.au}.
Comment: 17 pages, 8 figures
Databáze: OpenAIRE