| dc.date.accessioned | 2020-03-11T20:29:42Z | |
| dc.date.accessioned | 2022-10-18T22:47:25Z | |
| dc.date.available | 2020-03-11T20:29:42Z | |
| dc.date.available | 2022-10-18T22:47:25Z | |
| dc.date.created | 2020-03-11T20:29:42Z | |
| dc.date.issued | 2009 | |
| dc.identifier | http://hdl.handle.net/10533/238881 | |
| dc.identifier | 15010003 | |
| dc.identifier | WOS:000261982100011 | |
| dc.identifier | no scielo | |
| dc.identifier | eid=2-s2.0-58049184669 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4470220 | |
| dc.description.abstract | We study the reliability of the statistical background subtraction method for computing the Ks-band luminosity function of cluster galaxies at z∼ 1 using mock Red-sequence Cluster Survey cluster catalogues constructed from GALFORM semi-analytic galaxies. | |
| dc.language | eng | |
| dc.relation | https://doi.org/10.1111/j.1365-2966.2008.14059.x | |
| dc.relation | 10.1111/j.1365-2966.2008.14059.x | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.rights | Atribución-NoComercial-SinDerivadas 3.0 Chile | |
| dc.rights | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
| dc.title | On the accuracy of the high-redshift cluster luminosity function | |
| dc.type | Articulo | |
