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Closed Access item Near-Infrared galaxy counts and evolution from the wide-field Alhambra survey

Authors:Hornillos, Cristóbal
Molés, Mariano
Perea, Jaime
Castander, Francisco J.
Alfaro, Emilio J.
Benítez, Narciso
Cerviño, Miguel
Fernández-Soto, Alberto
González Delgado, Rosa M.
Husillos, César
Márquez, I.
Masegosa, J.
Olmo, Ascensión del
Prada, F.
Quintana, José María
Sánchez, Sebastián F.
Keywords:Cosmology: observations, Galaxies: evolution, Galaxies: high-redshift, Galaxies: photometry, Infrared: galaxies, Surveys
Issue Date:2009
Publisher:American Astronomical Society
Institute of Physics Publishing
Citation:Astrophysical Journal 696(2): 1554 (2009)
Abstract:The ALHAMBRA survey aims to cover 4 deg2 using a system of 20 contiguous, equal width, medium-band filters spanning the range 3500 Å-9700 Å plus the standard JHKs filters. Here we analyze deep near-IR number counts of one of our fields (ALH08) for which we have a relatively large area (0.5 deg2) and faint photometry (J = 22.4, H = 21.3, and K = 20.0 at the 50% of recovery efficiency for point-like sources). We find that the logarithmic gradient of the galaxy counts undergoes a distinct change to a flatter slope in each band: from 0.44 at [17.0, 18.5] to 0.34 at [19.5, 22.0] for the J band; for the H band 0.46 at [15.5, 18.0] to 0.36 at [19.0, 21.0], and in Ks the change is from 0.53 in the range [15.0, 17.0] to 0.33 in the interval [18.0, 20.0]. These observations together with faint optical counts are used to constrain models that include density and luminosity evolution of the local type-dependent luminosity functions. Our models imply a decline in the space density of evolved early-type galaxies with increasing redshift, such that only 30%-50% of the bulk of the present day red ellipticals was already in place at z~1.
Description:22 páginas, 32 figuras, 10 tablas.-- et al.
Publisher version (URL):http://dx.doi.org/10.1088/0004-637X/696/2/1554
URI:http://hdl.handle.net/10261/42448
ISSN:0004-637X
E-ISSNmetadata.dc.identifier.doi = DOI:1538-4357
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