[PDF] Top 20 Sunyaev zel'dovich effect observations of strong lensing galaxy clusters: probing the overconcentration problem

... in the LoCuSS sample. If the clusters in our sample have similarly low gas fractions compared to the LoCuSS sample, then the mass estimates we derive from the SZ scaling relation ... See full document

... galaxies, observations suggest that these galax- ies show some preference for residing in galaxy clusters (Coble et ...model of radio galaxies that describes their correlation with halos, ... See full document

... use the clusters’ optically derived properties to estimate photometric redshifts, optical luminosities, richness, and ...complement the optical measurements with archival XMM-Newton and ROSAT X-ray ... See full document

... densities of ∼10 − 5 Mpc −3 , consistent with optically selected quasars at z ∼ 2 and 2–3L ∗ elliptical galaxies at z ∼ 0 ...knowledge of SMGs has definitely advanced, their dominant formation mechanism is ... See full document

... Modelling the thrust-fault problem as a rigid-block pushed across a table is somewhat misleading because long-thin intact thrust sheets are in fact the exception rather than the ...1990). ... See full document

... thank the anonymous referee of this paper for useful com- ments that improved the ...manuscript. The CLASH Multi-Cycle Treasury Program (GO-12065) is based on observations made with ... See full document

... studies of the globular clusters located toward the center of the Milky Way have been historically ...neglected. The presence of patchy differential reddening in ... See full document

... on the final image stacks with the corresponding weight ...volve the data with a Gaussian kernel and require for a detection to have 4 contiguous pixels exceeding a S/N of ...on the ... See full document

... as the ratio mass/volume, so nondestructive probing methods are used to predict ...measurements. The goal of this paper is to study the influence of timber moisture content on ... See full document

... surpassed the number of galaxy–quasar lenses (more than 200 including COSMOS: Faure et ...when the number counts of lensed galaxies are, and will increasingly be, larger than lensed ... See full document

... surge of interest in cosmic voids is also partly thanks to a community that works on modified gravity theories (see ...for the latest reviews). This growing field explores the possibility that ... See full document

... contamination of the signal could remain, leading to an underestimate of the amplitude of the tSZ ...vary the level at which point sources are masked in the 218 GHz ... See full document

... as the use of RV measurements to improve the reliability of the KB, but any such approach would require the availability of additional data, ...scopic observations. ... See full document

... determine the flux and luminosity of each X-ray source, we used XSPEC 33 to model the instrument response within Posi- tion Sensitive Proportional Counter channels ...temperature of 8 keV and ... See full document

... is, of course, possible to boost the predicted number of contaminating objects to match the number of detected objects in the ACS field by arbitrarily increasing the ... See full document

... that the Arnaud et al. (2010) profile accurately describes the gas profiles of clusters in the MCXC and MaxBCG ...catalogs. The good agreement we find in Figure 4 and also shown ... See full document

... One of the strengths of our statistical analysis is that radio sources which are actually lobes of a central radio galaxy are included in the ...Mpc of the center ... See full document

... by the U.S. National Science Foundation through Grants AST-0408698 for the ACT project, and PHY-0355328, AST-0707731 and PIRE- 0507768 (Grant number ...OISE-0530095). The PIRE program made possible ... See full document

... thank the referee for the useful and construc- tive comments to improve this ...paper. The authors acknowledge support from Fondo ALMA-CONICYT N ◦ 31090019, Comité Mixto ESO-Gobierno de Chile, ... See full document

... selection effect by including 3 σ upper limits for spectroscopically con fi rmed infrared-detected cluster members above the scaling relation mass limit of 10 10 M ☉ ...each of these seven ... See full document