The clustering of the SDSS main galaxy sample – II. Mock galaxy catalogues and a measurement of the growth of structure from redshift space distortions at z = 0.15

By Cullan Howlett, A. Ross, L. Samushia, Will J. Percival, Marc Manera. 2014

235 citations recorded by the source corpus.

Citation: Howlett, C., Ross, A. J., Samushia, L., Percival, W. J., & Manera, M. (2015). The clustering of the SDSS main galaxy sample - II. Mock galaxy catalogues and a measurement of the growth of structure from redshift space distortions at z=0.15. Monthly Notices of the Royal Astronomical Society, 449(1), 848-866. doi:10.1093/mnras/stu2693

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/497eb8ae058bb6de0c33b53dc6398cf1fe68e1de

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Citations in the corpus

Tension and constraints on modified gravity parametrizations of $G_{\textrm{eff}}(z)$ from growth rate and Planck data (2017, background): “[69] Cullan Howlett, Ashley Ross, Lado Samushia, Will Percival, and Marc Manera, “The clustering of the SDSS main galaxy sample – II.”
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Constraining modified gravity (2016, methodology): “…BOSS data, we use RSD measurements from three different surveys (see Table 1): the SixDegree Field Galaxy Survey (6dFGS, Beutler et al. 2012), the SDSS Data Release 7 Main Galaxy Sample (MGS, Howlett et al. 2015) and the VIMOS Public Extragalactic Redshift Survey (VIPERS, de la Torre et al. 2013).”
The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1 (2020, methodology): “In our BAO analysis, we applied the reconstruction technique of Burden et al. (2014) and Burden, Percival & Howlett (2015) to the observed galaxy density field in order to remove a fraction of the RSDs, as well as non-linear motions of galaxies that smeared out the BAO peak.”
The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the quasar sample in configuration space between redshift 0.8 and 2.2 (2020, result): “We also show previous results from the SDSS main galaxy sample (MGS) for the distance measurement (Ross et al. 2015a) and growth rate measurement (Howlett et al. 2015), the constraints from BOSS DR12 LRG sample (Alam et al. 2017), and the combined constraints from eBOSS DR14 Lyα measurements (de…”
Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument (2023, methodology): “…on Ω Λ , H 0 , and σ 8 are possible when using the full sample of BAO and RSD measurements from the SDSS series of experiments (Ross et al. 2015; Howlett et al. 2015; Alam et al. 2017; Bautista et al. 2021; Gil-Mar´ın et al. 2020; Raichoor et al. 2021; Tamone et al. 2020; de Mattia et al.…”
Evolution of the f σ 8 tension with the Planck 15 / Λ CDM determination and implications for modified gravity theories (2018, background): “145 [89] 30 January 2015 (Ω0m, h, σ8) = (0.”
The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at z ∼ 1.4 (2015, background): “These constraints include the studies of the 6dFGS (Beutler et al. 2012), the SDSS main galaxies (Howlett et al. 2015), the 2dFGRS (Song & Percival 2009), the SDSS LRG (Samushia et al. 2012), the BOSS LOWZ (Chuang et al. 2013), the BOSS CMASS (Reid et al. 2012), WiggleZ (Blake et al. 2011), VVDS…”
Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory (2020, methodology): “The sample was used to perform a BAO measurement from the recon- 4 http://sdss.physics.nyu.edu/vagc/lss.html structed correlation function (Ross et al. 2015) and an RSD measurement from the anisotropic correlation function (Howlett et al. 2015), both at an effective redshift zeff = 0.15.”
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample (2016, methodology): “…6dFGS (Beutler et al. 2012), GAMA (Blake et al. 2013), WiggleZ (Blake et al. 2012), VVDS (Guzzo et al. 2008), and VIPERS (de la Torre et al. 2013), as well as the measurements from the SDSS-I and -II main galaxy sample (Howlett et al. 2015, MGS) and the SDSS-II LRG sample (Oka et al. 2014, DR7).”
Planck2015 results (2015, unknown): “Neglecting the AP effect can lead to biased measurements of fσ8 if the assumed cosmology differs, and to significant underestimation of the errors (Howlett et al. 2015).”