Deconstructing the K-band number counts
| dc.contributor.author | Barro, Guillermo | |
| dc.contributor.author | Gallego Maestro, Jesús | |
| dc.contributor.author | Pérez González, Pablo Guillermo | |
| dc.contributor.author | Eliche Moral, María del Carmen | |
| dc.contributor.author | Balcells, M. | |
| dc.contributor.author | Villar, V. | |
| dc.contributor.author | Cardiel López, Nicolás | |
| dc.contributor.author | Cristobal Hornillos, D. | |
| dc.contributor.author | Gil De Paz, Armando | |
| dc.contributor.author | Guzmán, R. | |
| dc.contributor.author | Pelló, R. | |
| dc.contributor.author | Prieto, M. | |
| dc.contributor.author | Zamorano Calvo, Jaime | |
| dc.date.accessioned | 2023-06-20T00:48:31Z | |
| dc.date.available | 2023-06-20T00:48:31Z | |
| dc.date.issued | 2010 | |
| dc.description | © Springer-Verlag Berlin Heidelberg 2010. Scientific Meeting of the Spanish-Astronomical-Society (SEA) (8th; 2008; Santander-SPAIN) | |
| dc.description.abstract | We present a study that links the NCs to the rest-frame luminosity functions (LFs) at the passbands probed by the observed K-band at different epochs. Making use of a large K-band selected sample in the Groth Field, HDFN and CDFS (∼0.27deg^(2)), we have derived highly reliable photometric redshift estimates that allow us to estimate LFs in the redshift range [0.25-1.25]. We find that the larger flattening in the slope of the K-band NCs is mostly a consequence of a prominent decrease in the characteristic density (φ∗) around z∼1, and an almost flat evolution of M∗. | |
| dc.description.department | Depto. de Física de la Tierra y Astrofísica | |
| dc.description.faculty | Fac. de Ciencias Físicas | |
| dc.description.refereed | TRUE | |
| dc.description.status | pub | |
| dc.eprint.id | https://eprints.ucm.es/id/eprint/59841 | |
| dc.identifier.doi | 10.1007/978-3-642-11250-8_29 | |
| dc.identifier.issn | 1570-6591 | |
| dc.identifier.officialurl | http://dx.doi.org/10.1007/978-3-642-11250-8_29 | |
| dc.identifier.relatedurl | https://link.springer.com/ | |
| dc.identifier.uri | https://hdl.handle.net/20.500.14352/43001 | |
| dc.journal.title | Highlights of Spanich Astrophysics | |
| dc.language.iso | eng | |
| dc.page.final | 259 | |
| dc.page.initial | 259 | |
| dc.publisher | Springer-Verlag Berlin | |
| dc.rights.accessRights | restricted access | |
| dc.subject.cdu | 52 | |
| dc.subject.keyword | Astronomy | |
| dc.subject.keyword | Astrophysics | |
| dc.subject.ucm | Astrofísica | |
| dc.title | Deconstructing the K-band number counts | |
| dc.type | journal article | |
| dspace.entity.type | Publication | |
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| relation.isAuthorOfPublication.latestForDiscovery | 303794a4-e4bf-4262-9a94-11bc46167d8e |
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