On the nature of the extragalactic number counts in the K-band

dc.contributor.authorBarro, G.
dc.contributor.authorGallego Maestro, Jesús
dc.contributor.authorPérez González, Pablo Guillermo
dc.contributor.authorEliche Moral, María del Carmen
dc.contributor.authorBalcells, M.
dc.contributor.authorVillar, V.
dc.contributor.authorCardiel López, Nicolás
dc.contributor.authorCristobal Hornillos, D.
dc.contributor.authorGil de Paz, Armando
dc.contributor.authorGuzmán, R.
dc.contributor.authorPello, R.
dc.contributor.authorPrieto, M.
dc.contributor.authorZamorano Calvo, Jaime
dc.date.accessioned2023-06-20T03:47:46Z
dc.date.available2023-06-20T03:47:46Z
dc.date.issued2009-01
dc.description© ESO 2009. We thank the referee M. Bershady for his useful and constructive comments. We acknowledge support from the Spanish Programa Nacional de Astronomía y Astrofísica under grant AYA 2006-02358. Partially funded by the Spanish MEC under the Consolider-Ingenio 2010 Program grant CSD2006-00070: First Science with the GTC (http://www.iac.es/consolider-ingenio-gtc/). Based on observations collected at the Centro Astronómico Hispano Alemán (CAHA) at Calar Alto, operated jointly by the Max-Planck Institut fur Astronomie and the Instituto de Astrofísica de Andalucía (CSIC). This article is based on observations made with the WHT operated on the island of La Palma by the Instituto Astrofísico de Canarias in the Spanish Observatorio del Roque de los Muchachos. This work is based in part on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, Caltech under NASA contract 1407. GALEX is a NASA Small Explorer launched in 2003 April. We gratefully acknowledge NASA's support for construction, operation, and scientific analysis of the GALEX mission. Based in part on data collected at Subaru Telescope and obtained from the SMOKA, which is operated by the Astronomy Data Center, National Astronomical Observatory of Japan. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii.
dc.description.abstractContext. The galaxy number counts has been traditionally used to test models of galaxy evolution. However, the origin of significant differences in the shape of number counts at different wavelengths is still unclear. By relating the most remarkable features in the number counts with the underlying galaxy population it is possible to introduce further constraints on galaxy evolution. Aims. We aim to investigate the causes of the different shape of the K-band number counts when compared to other bands, analyzing in detail the presence of a change in the slope around K similar to 17.5. Methods. We present a near-infrared imaging survey, conducted at the 3.5 m telescope of the Calar Alto Spanish-German Astronomical Center (CAHA), covering two separated fields centered on the HFDN and the Groth field, with a total combined area of similar to 0.27 deg(2) to a depth of K similar to 19 (3 sigma, Vega). By combining our data with public deep K-band images in the CDFS (GOODS/ISAAC) and high quality imaging in multiple bands, we extract K-selected catalogs characterized with highly reliable photometric redshift estimates. We derive redshift binned number counts, comparing the results in our three fields to sample the effects of cosmic variance. We derive luminosity functions from the observed K-band in the redshift range [0.25-1.25], that are combined with data from the references in multiple bands and redshifts, to build up the K-band number count distribution. Results. The overall shape of the number counts can be grouped into three regimes: the classic Euclidean slope regime (d log N/dm similar to 0.6) at bright magnitudes; a transition regime at intermediate magnitudes, dominated by M* galaxies at the redshift that maximizes the product phi*dVc/d Omega; and an alpha dominated regime at faint magnitudes, where the slope asymptotically approaches -0.4(alpha + 1) controlled by post-M* galaxies. The slope of the K-band number counts presents an averaged decrement of similar to 50% in the range 15.5 < K < 18.5 (d log N/dm similar to 0.6-0.30). The rate of change in the slope is highly sensitive to cosmic variance effects. The decreasing trend is the consequence of a prominent decrease of the characteristic density phi(K,obs)* (similar to 60% from z = 0.5 to z = 1.5) and an almost flat evolution of M(K,obs)* (1 sigma compatible with M(K,obs)* = -22.89 +/- 0.25 in the same redshift range).
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipSpanish Programa Nacional de Astronomia y Astrofísica
dc.description.sponsorshipSpanish MEC
dc.description.sponsorshipNASA
dc.description.sponsorshipNational Astronomical Observatory of Japan
dc.description.sponsorshipNational Science Foundation
dc.description.sponsorshipCanada-France-Hawaii Telescope (CFHT)
dc.description.sponsorshipNational Research Council (NRC) of Canada
dc.description.sponsorshipInstitut National des Science de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France
dc.description.sponsorshipUniversity of Hawaii
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/28096
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dc.identifier.doi10.1051/0004-6361:200810633
dc.identifier.issn0004-6361
dc.identifier.officialurlhttp://dx.doi.org/10.1051/0004-6361:200810633
dc.identifier.relatedurlhttp://www.aanda.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/44457
dc.issue.number1
dc.journal.titleAstronomy & Astrophysics
dc.language.isoeng
dc.page.final79
dc.page.initial63
dc.publisherEDP Sciencies
dc.relation.projectIDAYA 2006-02358
dc.relation.projectIDCSD2006-00070
dc.relation.projectIDNASA contract 1407
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordGalaxy luminosity function
dc.subject.keywordDeep-field-south
dc.subject.keywordSpectral energy-distributions
dc.subject.keywordActive galactic nuclei
dc.subject.keywordEarly data release
dc.subject.keywordGoods-North field
dc.subject.keywordYale-Chile musyc
dc.subject.keyword1st epoch data
dc.subject.keywordRedshift survey
dc.subject.keywordMulti wavelength survey
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.subject.ucmFísica atmosférica
dc.subject.unesco2501 Ciencias de la Atmósfera
dc.titleOn the nature of the extragalactic number counts in the K-band
dc.typejournal article
dc.volume.number494
dspace.entity.typePublication
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