Sunyaev-Zel'dovich power spectrum and cluster numbers from an extended merger-tree model

Irina Dvorkin*, Yoel Rephaeli, Meir Shimon

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

4 Scopus citations


We have recently developed an extended merger-tree model that efficiently follows hierarchical evolution of galaxy clusters and provides a quantitative description of both their dark matter and gas properties. We employed this diagnostic tool to calculate the thermal Sunyaev-Zel'dovich power spectrum and cluster number counts, accounting explicitly for uncertainties in the relevant statistical and intrinsic cluster properties, such as the halo mass function and the gas equation of state. Results of these calculations are compared with those obtained from a direct analytic treatment and from hydrodynamical simulations. We show that under certain assumptions on the gas mass fraction our results are consistent with the latest South Pole Telescope measurement. Our approach can be particularly useful in predicting cluster number counts and their dependence on cluster and cosmological parameters.

Original languageEnglish
Pages (from-to)2648-2655
Number of pages8
JournalMonthly Notices of the Royal Astronomical Society
Issue number3
StatePublished - Apr 2012


  • Cosmic background radiation
  • Galaxies: clusters: general
  • Large-scale structure of Universe


Dive into the research topics of 'Sunyaev-Zel'dovich power spectrum and cluster numbers from an extended merger-tree model'. Together they form a unique fingerprint.

Cite this