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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/25317
Title: Galaxy clusters as probes for cosmology and dark matter
Authors: Battistelli, Elia S.
BURIGANA, CARLO 
De Bernardis, Paolo
Kirillov, Alexander A.
Neto, Gastao B. Lima
Masi, Silvia
Norgaard-Nielsen, Hans U.
Ostermann, Peter
Roman, Matthieu
Rosati, Piero
ROSSETTI, MARIACHIARA 
Issue Date: 2016
Journal: INTERNATIONAL JOURNAL OF MODERN PHYSICS D 
Number: 25
Issue: 10
First Page: 1630023
Abstract: In recent years, significant progress has been made in building new galaxy clusters samples, at low and high redshifts, from wide-area surveys, particularly exploiting the Sunyaev-Zel’dovich (SZ) effect. A large effort is underway to identify and characterize these new systems with optical/NIR and X-ray facilities, thus opening new avenues to constraint cosmological models using structure growth and geometrical tests. A census of galaxy clusters sets constraints on reionization mechanisms and epochs, which need to be reconciled with recent limits on the reionization optical depth from cosmic microwave background (CMB) experiments. Future advances in SZ effect measurements will include the possibility to (unambiguously) measure directly the kinematic SZ effect, to build an even larger catalogue of galaxy clusters able to study the high redshift universe, and to make (spatially-)resolved galaxy cluster maps with even spectral capability to (spectrally-)resolve the relativistic corrections of the SZ effect.
URI: http://hdl.handle.net/20.500.12386/25317
URL: https://www.worldscientific.com/doi/abs/10.1142/S0218271816300238
https://arxiv.org/pdf/1609.01110.pdf
ISSN: 0218-2718
DOI: 10.1142/S0218271816300238
Bibcode ADS: 2016IJMPD..2530023B
Fulltext: open
Appears in Collections:1.01 Articoli in rivista

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