Hostname: page-component-68945f75b7-6q656 Total loading time: 0 Render date: 2024-09-03T13:47:25.012Z Has data issue: false hasContentIssue false
  • English
  • Français

Constraints on radio source clustering towards galaxy clusters: application for cm-wavelength simulations of blind sky surveys

Published online by Cambridge University Press:  12 October 2016

Bartosz Lew
Bartosz Lew*
Affiliation:
Toruń Centre for Astronomy, Nicolaus Copernicus University, ul. Gagarina 11, 87-100 Toruń, Poland email: blew@astro.uni.torun.pl
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We derive constraints on radio source clustering towards Planck-selected galaxy clusters using the NVSS point source catalog. The constraint can be used for making a more realistic Sunyaev-Zeldovich effect (SZE) mocks, calculating predictions of detectable clusters count and for quantifying source confusion in radio surveys.

Keywords

SZEcosmological simulationsgalaxy clustersradio surveys
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S308: The Zeldovich Universe: Genesis and Growth of the Cosmic Web , June 2014 , pp. 301 - 302
Copyright
Copyright © International Astronomical Union 2016 

References

Coble, K., et al. 2007, AJ 897, 134 [astro-ph/0608274]Google Scholar
Condon, J. J., et al. 1998, AJ 1693–1716, 115 Google Scholar
Lew, B., et al. 2014, submitted to JCAP [arxiv:1410:3660]Google Scholar
Planck Collaboration: Ade, P. A. R., et al. 2011, A&A A8, 536 [arxiv:1101.2024]Google Scholar
Planck Collaboration: Ade, P. A. R., et al. 2014, A&A accepted [arxiv:1303.5062]Google Scholar