Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26539
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Sereno, Mauro | en_US |
dc.contributor.author | COVONE, GIOVANNI | en_US |
dc.contributor.author | IZZO, LUCA | en_US |
dc.contributor.author | ETTORI, STEFANO | en_US |
dc.contributor.author | Coupon, Jean | en_US |
dc.contributor.author | Lieu, Maggie | en_US |
dc.date.accessioned | 2020-07-21T06:37:23Z | - |
dc.date.available | 2020-07-21T06:37:23Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26539 | - |
dc.description.abstract | The possibly unbiased selection process in surveys of the Sunyaev Zel'dovich effect can unveil new populations of galaxy clusters. We performed a weak lensing analysis of the PSZ2LenS sample, i.e. the PSZ2 galaxy clusters detected by the Planck mission in the sky portion covered by the lensing surveys CFHTLenS and RCSLenS. PSZ2LenS consists of 35 clusters and it is a statistically complete and homogeneous subsample of the PSZ2 catalogue. The Planck selected clusters appear to be unbiased tracers of the massive end of the cosmological haloes. The mass-concentration relation of the sample is in excellent agreement with predictions from the Λ cold dark matter model. The stacked lensing signal is detected at 14σ significance over the radial range 0.1 < R < 3.2 Mpc h<SUP>-1</SUP>, and is well described by the cuspy dark halo models predicted by numerical simulations. We confirmed that Planck estimated masses are biased low by b<SUB>SZ</SUB> = 27 ± 11(stat) ± 8(sys) per cent with respect to weak lensing masses. The bias is higher for the cosmological subsample, b<SUB>SZ</SUB> = 40 ± 14(stat) ± 8(sys) per cent. | en_US |
dc.language.iso | eng | en_US |
dc.title | PSZ2LenS. Weak lensing analysis of the Planck clusters in the CFHTLenS and in the RCSLenS | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stx2085 | en_US |
dc.identifier.scopus | 2-s2.0-85040835957 | en_US |
dc.identifier.isi | 000413082900054 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article-abstract/472/2/1946/4082237 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 472 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 1946 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 6 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | en_US |
dc.identifier.adsbibcode | 2017MNRAS.472.1946S | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_6 Stars and stellar systems | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0003-0302-0325 | - |
crisitem.author.orcid | 0000-0003-4117-8617 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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stx2085.pdf | PDF editoriale | 3.15 MB | Adobe PDF | View/Open |
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