Velocity dispersion and dynamical masses for 388 Galaxy Clusters and groups. Calibrating the -- scaling relation for the PSZ2 sample
arXiv:2111.13071 · doi:10.1051/0004-6361/202039980
Abstract
The second catalogue of Planck Sunyaev-Zeldovich (SZ) sources, hereafter PSZ2, represents the largest galaxy cluster sample selected by means of their SZ signature in a full-sky survey. Using telescopes at the Canary Island observatories, we conducted the long-term observational program 128- MULTIPLE-16/15B (hereafter LP15), a large and complete optical follow-up campaign of all the unidentified PSZ2 sources in the northern sky, with declinations above and no correspondence in the first Planck catalogue PSZ1. This paper is the third and last in the series of LP15 results, after Streblyanska et al. (2019) and Aguado-Barahona et al. (2019), and presents all the spectroscopic observations of the full program. We complement these LP15 spectroscopic results with Sloan Digital Sky Survey (SDSS) archival data and other observations from a previous program (ITP13-08), and present a catalog of 388 clusters and groups of galaxies including estimates of their velocity dispersion. The majority of them (356) are the optical counterpart of a PSZ2 source. A subset of 297 of those clusters is used to construct the scaling relation, based on the estimated SZ mass from Planck measurements and our dynamical mass estimates. We discuss and correct for different statistical and physical biases in the estimation of the masses, such as the Eddington bias when estimating and the aperture and the number of galaxies used to calculate . The SZ-to-dynamical mass ratio for those 297 PSZ2 clusters is (stat) (sys), with only marginal evidence for a possible mass dependence of this factor. Our value is consistent with previous results in the literature, but presents a significantly smaller uncertainty due to the use of the largest sample size for this type of studies.
21 pages, 7 figures. Accepted for publication
References in corpus (11)
- Some Aspects of Measurement Error in Linear Regression of Astronomical Data
- Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
- The Canadian Cluster Comparison Project: detailed study of systematics and updated weak lensing masses
- The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
- The relation between velocity dispersion and mass in simulated clusters of galaxies: dependence on the tracer and the baryonic physics
- The universal distribution of halo interlopers in projected phase space. Bias in galaxy cluster concentration and velocity anisotropy?
- Galaxy Cluster Mass Reconstruction Project: I. Methods and first results on galaxy-based techniques
- Planck Sunyaev-Zel'dovich Cluster Mass Calibration using Hyper Suprime-Cam Weak Lensing
- Biases in galaxy cluster velocity dispersion and mass estimates in the small number of galaxies regime
- Velocity dispersion and dynamical mass for 270 galaxy clusters in the Planck PSZ1 catalogue
- Optical validation and characterisation of Planck PSZ1 sources at the Canary Islands observatories. II. Second year of ITP13 observations
Cited by in corpus (12)
- Multi-probe analysis of the galaxy cluster CL J1226.9+3332: Hydrostatic mass and hydrostatic-to-lensing bias
- Marginalised Normal Regression: Unbiased curve fitting in the presence of x-errors
- XLSSC 122 caught in the act of growing up: Spatially resolved SZ observations of a z=1.98 galaxy cluster
- Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
- Virial theorem in clusters of galaxies with MOND
- Examining the local Universe isotropy with galaxy cluster velocity dispersion scaling relations
- The hydrostatic-to-lensing mass bias from resolved X-ray and optical-IR data
- Mass bias and cosmological constraints from Planck cluster clustering
- CHEX-MATE: exploring the kinematical properties of Planck galaxy clusters
- Unveiling the shape: a multi-wavelength analysis of the galaxy clusters Abell 76 and Abell 1307
- Galaxy cluster mass bias from projected mass maps: The Three Hundred-NIKA2 LPSZ twin samples
- A Spectroscopic View of the JWST/GTO Strong Lensing Cluster A1489