SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV - Archive ouverte HAL Access content directly
Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2016

SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV

, , , , , , , , (1) , , , , , , , , , , ,
1
N. Clerc
A. Merloni
  • Function : Author
Y. -Y. Zhang
  • Function : Author
A. Finoguenov
T. Dwelly
  • Function : Author
K. Nandra
  • Function : Author
C. Collins
  • Function : Author
K. Dawson
  • Function : Author
E. Rozo
  • Function : Author
E. Rykoff
  • Function : Author
T. Sadibekova
  • Function : Author
J. Brownstein
  • Function : Author
Y. -T. Lin
  • Function : Author
J. Ridl
  • Function : Author
M. Salvato
  • Function : Author
A. Schwope
  • Function : Author
M. Steinmetz
  • Function : Author
H. -J. Seo
  • Function : Author
J. Tinker
  • Function : Author

Abstract

SPIDERS (The SPectroscopic IDentification of eROSITA Sources) is a programme dedicated to the homogeneous and complete spectroscopic follow-up of X-ray active galactic nuclei and galaxy clusters over a large area (∼7500 deg2) of the extragalactic sky. SPIDERS is part of the Sloan Digital Sky Survey (SDSS)-IV project, together with the Extended Baryon Oscillation Spectroscopic Survey and the Time-Domain Spectroscopic Survey. This paper describes the largest project within SPIDERS before the launch of eROSITA: an optical spectroscopic survey of X-ray-selected, massive (∼1014-1015 M) galaxy clusters discovered in ROSAT and XMM-Newton imaging. The immediate aim is to determine precise (Δz ∼ 0.001) redshifts for 4000-5000 of these systems out to z ∼ 0.6. The scientific goal of the program is precision cosmology, using clusters as probes of large-scale structure in the expanding Universe. We present the cluster samples, target selection algorithms and observation strategies. We demonstrate the efficiency of selecting targets using a combination of SDSS imaging data, a robust red-sequence finder and a dedicated prioritization scheme. We describe a set of algorithms and work-flow developed to collate spectra and assign cluster membership, and to deliver catalogues of spectroscopically confirmed clusters. We discuss the relevance of line-of-sight velocity dispersion estimators for the richer systems. We illustrate our techniques by constructing a catalogue of 230 spectroscopically validated clusters (0.031 < z < 0.658), found in pilot observations. We discuss two potential science applications of the SPIDERS sample: the study of the X-ray luminosity-velocity dispersion (LX-σ) relation and the building of stacked phase-space diagrams.
Fichier principal
Vignette du fichier
stw2214.pdf (12.67 Mo) Télécharger le fichier
Origin : Publisher files allowed on an open archive

Dates and versions

insu-03667682 , version 1 (13-05-2022)

Identifiers

Cite

N. Clerc, A. Merloni, Y. -Y. Zhang, A. Finoguenov, T. Dwelly, et al.. SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV. Monthly Notices of the Royal Astronomical Society, 2016, 463, pp.4490-4515. ⟨10.1093/mnras/stw2214⟩. ⟨insu-03667682⟩
48 View
3 Download

Altmetric

Share

Gmail Facebook Twitter LinkedIn More