Astrophysical Journal

dc.creatorGralla, M.
dc.creatorBarrientos, L.F.
dc.date2019-12-18T18:15:09Z
dc.date2022-07-07T23:39:46Z
dc.date2019-12-18T18:15:09Z
dc.date2022-07-07T23:39:46Z
dc.date2011
dc.date.accessioned2023-08-21T20:51:01Z
dc.date.available2023-08-21T20:51:01Z
dc.identifier15010003
dc.identifier15010003
dc.identifierhttps://hdl.handle.net/10533/237273
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8280727
dc.descriptionWe have measured the Sunyaev Zel'dovich (SZ) effect for a sample of ten strong lensing selected galaxy clusters using the Sunyaev Zel'dovich Array (SZA). The SZA is sensitive to structures on spatial scales of a few arcminutes, while the strong lensing mass modeling constrains the mass at small scales (typically < 30"). Combining the two provides information about the projected concentrations of the strong lensing clusters. The Einstein radii we measure are twice as large as expected given the masses inferred from SZ scaling relations. A Monte Carlo simulation indicates that a sample randomly drawn from the expected distribution would have a larger median Einstein radius than the observed clusters about 3% of the time. The implied overconcentration has been noted in previous studies with smaller samples of lensing clusters. It persists for this sample, with the caveat that this could result from a systematic effect such as if the gas fractions of the strong lensing clusters are substantially below what is expected.
dc.descriptionFONDAP
dc.descriptionFONDAP
dc.languageeng
dc.relationinstname: Conicyt
dc.relationreponame: Repositorio Digital RI2.0
dc.relationinfo:eu-repo/grantAgreement/Fondap/15010003
dc.relationhttps://arxiv.org/abs/1011.6341
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleSunyaev-Zel'dovich Effect Observations of Strong Lensing Galaxy Clusters: Probing the Overconcentration Problem
dc.titleAstrophysical Journal
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


Este ítem pertenece a la siguiente institución