Batch discovery of nine <i>z</i> ∼ 1 clusters using X-ray and <i>K</i> or <i>R</i>, <i>z</i>′ images
dc.contributor.author | Andreon, S | |
dc.contributor.author | Valtchanov, I | |
dc.contributor.author | Jones, LR | |
dc.contributor.author | Altieri, B | |
dc.contributor.author | Bremer, M | |
dc.contributor.author | Willis, J | |
dc.contributor.author | Pierre, M | |
dc.contributor.author | Quintana, H | |
dc.date.accessioned | 2025-01-21T01:06:54Z | |
dc.date.available | 2025-01-21T01:06:54Z | |
dc.date.issued | 2005 | |
dc.description.abstract | We present the results of an initial search for clusters of galaxies at z similar to 1 and above, using data from 2.9 square degrees of XMM-Newton images. By selecting weak potentially extended X-ray sources with faint or no identifications in deep, ground-based optical imaging, we have constructed a starting sample of 19 high-redshift cluster candidates. Near-IR and R, z' imaging of these fields identified nine of them as high-redshift systems. Six of these were confirmed spectroscopically, three at z similar to 1.0 and the other three in the 0.8 < Z < 0.92 range. The remaining three systems have solid photometric evidence to be at Z(phot) similar to 0-8, 1.0 and 1.3. The present sample significantly increases the number of such clusters. The measured density of z I clusters, after discarding 'low'-redshift systems at z less than or similar to 0.92 is about 1.7 deg(-2) (with 68 per cent confidence interval equal to [1.0, 2.9]) for f(x) greater than or similar to 2.5 10(-15) erg cm(-2) s(-1) ([0.5-2] keV) and this is a lower limit, having, screened not all potential z similar to 1 candidate clusters. Coordinates, X-ray measures and evidence for nine X-ray-selected high-redshift clusters is given. | |
dc.fuente.origen | WOS | |
dc.identifier.doi | 10.1111/j.1365-2966.2005.08998.x | |
dc.identifier.eissn | 1365-2966 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.uri | https://doi.org/10.1111/j.1365-2966.2005.08998.x | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/96242 | |
dc.identifier.wosid | WOS:000229640600005 | |
dc.issue.numero | 4 | |
dc.language.iso | en | |
dc.pagina.final | 1260 | |
dc.pagina.inicio | 1250 | |
dc.revista | Monthly notices of the royal astronomical society | |
dc.rights | acceso restringido | |
dc.subject | galaxies : clusters : general | |
dc.subject | cosmology : observations | |
dc.subject | X-rays : galaxies : clusters | |
dc.title | Batch discovery of nine <i>z</i> ∼ 1 clusters using X-ray and <i>K</i> or <i>R</i>, <i>z</i>′ images | |
dc.type | artículo | |
dc.volumen | 359 | |
sipa.index | WOS | |
sipa.trazabilidad | WOS;2025-01-12 |