TY - JOUR
T1 - High redshift galaxies in the ALHAMBRA survey I. Selection method and number counts based on redshift PDFs
AU - Viironen, K.
AU - Marin-Franch, A.
AU - Lopez-Sanjuan, C.
AU - Varela, J.
AU - Chaves-Montero, J.
AU - Cristobal-Hornillos, D.
AU - Molino, A.
AU - Fernandez-Soto, A.
AU - Vilella-Rojo, G.
AU - Ascaso, B.
AU - Cenarro, A. J.
AU - Cervino, M.
AU - Cepa, J.
AU - Ederoclite, A.
AU - Marquez, I.
AU - Masegosa, J.
AU - Moles, M.
AU - Oteo, I.
AU - Povic, M.
AU - Aguerri, J. A. L.
AU - Alfaro, E.
AU - Aparicio-Villegas, T.
AU - Benitez, N.
AU - Broadhurst, T.
AU - Cabrera-Cano, J.
AU - Castander, J. F.
AU - Del Olmo, A.
AU - Gonzalez Delgado, R. M.
AU - Husillos, C.
AU - Infante, L.
AU - Martinez, V. J.
AU - Perea, J.
AU - Prada, F.
AU - Quintana, J. M.
PY - 2015/4
Y1 - 2015/4
N2 - Context. Most observational results on the high redshift restframe UV-bright galaxies are based on samples pinpointed using the so-called dropout technique or Ly-alpha selection. However, the availability of multifilter data now allows the dropout selections to be replaced by direct methods based on photometric redshifts. In this paper we present the methodology to select and study the population of high redshift galaxies in the ALHAMBRA survey data.Aims. Our aim is to develop a less biased methodology than the traditional dropout technique to study the high redshift galaxies in ALHAMBRA and other multifilter data. Thanks to the wide area ALHAMBRA covers, we especially aim at contributing to the study of the brightest, least frequent, high redshift galaxies.Methods. The methodology is based on redshift probability distribution functions (zPDFs). It is shown how a clean galaxy sample can be obtained by selecting the galaxies with high integrated probability of being within a given redshift interval. However, reaching both a complete and clean sample with this method is challenging. Hence, a method to derive statistical properties by summing the zPDFs of all the galaxies in the redshift bin of interest is introduced.Results. Using this methodology we derive the galaxy rest frame UV number counts in five redshift bins centred at z = 2.5, 3.0, 3.5, 4.0, and 4.5, being complete up to the limiting magnitude at mUV(AB) = 24, where mUV refers to the first ALHAMBRA filter redwards of the Ly-alpha line. With the wide field ALHAMBRA data we especially contribute to the study of the brightest ends of these counts, accurately sampling the surface densities down to mUV(AB) = 21-22.Conclusions. We show that using the zPDFs it is easy to select a very clean sample of high redshift galaxies. We also show that it is better to do statistical analysis of the properties of galaxies using a probabilistic approach, which takes into account both the incompleteness and contamination issues in a natural way.
AB - Context. Most observational results on the high redshift restframe UV-bright galaxies are based on samples pinpointed using the so-called dropout technique or Ly-alpha selection. However, the availability of multifilter data now allows the dropout selections to be replaced by direct methods based on photometric redshifts. In this paper we present the methodology to select and study the population of high redshift galaxies in the ALHAMBRA survey data.Aims. Our aim is to develop a less biased methodology than the traditional dropout technique to study the high redshift galaxies in ALHAMBRA and other multifilter data. Thanks to the wide area ALHAMBRA covers, we especially aim at contributing to the study of the brightest, least frequent, high redshift galaxies.Methods. The methodology is based on redshift probability distribution functions (zPDFs). It is shown how a clean galaxy sample can be obtained by selecting the galaxies with high integrated probability of being within a given redshift interval. However, reaching both a complete and clean sample with this method is challenging. Hence, a method to derive statistical properties by summing the zPDFs of all the galaxies in the redshift bin of interest is introduced.Results. Using this methodology we derive the galaxy rest frame UV number counts in five redshift bins centred at z = 2.5, 3.0, 3.5, 4.0, and 4.5, being complete up to the limiting magnitude at mUV(AB) = 24, where mUV refers to the first ALHAMBRA filter redwards of the Ly-alpha line. With the wide field ALHAMBRA data we especially contribute to the study of the brightest ends of these counts, accurately sampling the surface densities down to mUV(AB) = 21-22.Conclusions. We show that using the zPDFs it is easy to select a very clean sample of high redshift galaxies. We also show that it is better to do statistical analysis of the properties of galaxies using a probabilistic approach, which takes into account both the incompleteness and contamination issues in a natural way.
KW - galaxies: evolution
KW - galaxies: distances and redshifts
KW - galaxies: high-redshift
KW - galaxies: statistics
KW - LYMAN-BREAK GALAXIES
KW - STAR-FORMING GALAXIES
KW - REST-FRAME ULTRAVIOLET
KW - SUBARU DEEP FIELDS
KW - PHOTOMETRIC REDSHIFT
KW - SPECTROSCOPIC SURVEY
KW - DATA RELEASE
KW - LUMINOSITY FUNCTIONS
KW - FORMATION RATES
KW - STELLAR MASSES
U2 - 10.1051/0004-6361/201425382
DO - 10.1051/0004-6361/201425382
M3 - Article
SN - 0004-6361
VL - 576
JO - Astronomy & Astrophysics
JF - Astronomy & Astrophysics
M1 - 25
ER -