Photometric redshifts and cluster tomography in the ESO Distant Cluster Survey

Context. This paper reports the results obtained on the photometric redshifts measurement and accuracy, and cluster tomography in the ESO Distant Cluster Survey (EDisCS) fields.

[1]  R. Pelló,et al.  THE REST-FRAME OPTICAL LUMINOSITY FUNCTION OF CLUSTER GALAXIES AT z < 0.8 AND THE ASSEMBLY OF THE CLUSTER RED SEQUENCE , 2009, 0905.4503.

[2]  D. Thompson,et al.  COSMOS PHOTOMETRIC REDSHIFTS WITH 30-BANDS FOR 2-deg2 , 2008, 0809.2101.

[3]  Edinburgh,et al.  The evolution of the brightest cluster galaxies since z∼ 1 from the ESO Distant Cluster Survey (EDisCS) , 2008, 0804.2152.

[4]  Luc Simard,et al.  Spectroscopy of clusters in the ESO distant cluster survey (EDisCS). II. - Redshifts, velocity dispersions, and substructure for clusters in the last 15 fields , 2008, 0802.0149.

[5]  N. Benı́tez,et al.  A blind test of photometric redshifts on ground-based data , 2008, 0801.2975.

[6]  H. Yee,et al.  FINDING GALAXY GROUPS IN PHOTOMETRIC-REDSHIFT SPACE: THE PROBABILITY FRIENDS-OF-FRIENDS ALGORITHM , 2008, 0801.2410.

[7]  Manda Banerji,et al.  Photometric Redshifts for the Dark Energy Survey and VISTA and Implications for Large Scale Structure , 2007, 0711.1059.

[8]  D. Wittman,et al.  Photometric Redshifts and Signal-to-Noise Ratios , 2007, 0707.2403.

[9]  D. Schiminovich,et al.  The First Release COSMOS Optical and Near-IR Data and Catalog , 2007, 0704.2430.

[10]  R. Pelló,et al.  The Morphological Content of 10 EDisCS Clusters at 0.5 < z < 0.8 , 2007, astro-ph/0701788.

[11]  D. Thompson,et al.  Photometric Redshifts of Galaxies in COSMOS , 2006, astro-ph/0612344.

[12]  R. Pelló,et al.  The build-up of the colour-magnitude relation in galaxy clusters since z ~ 0.8 , 2006, astro-ph/0610373.

[13]  D. Thompson,et al.  The Zurich Extragalactic Bayesian Redshift Analyzer and its first application: COSMOS , 2006, astro-ph/0609044.

[14]  R. Pelló,et al.  The X-ray properties of optically selected z > 0.6 clusters in the European Southern Observatory Distant Cluster Survey , 2006, astro-ph/0607662.

[15]  R. Bouwens,et al.  Galaxies in the Hubble Ultra Deep Field. I. Detection, Multiband Photometry, Photometric Redshifts, and Morphology , 2006, astro-ph/0605262.

[16]  B. Garilli,et al.  Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey , 2006, astro-ph/0603217.

[17]  R. Pelló,et al.  The Evolution of the Star Formation Activity in Galaxies and Its Dependence on Environment , 2005, astro-ph/0512391.

[18]  R. Pelló,et al.  Weak lensing mass reconstructions of the ESO distant cluster survey , 2005, astro-ph/0511746.

[19]  Y. Mellier,et al.  EDisCS - the ESO distant cluster survey. Sample definition and optical photometry , 2005, astro-ph/0508351.

[20]  Donald W. McCarthy, Jr.,et al.  Hα-derived Star Formation Rates for Three z≃0.75 EDisCS Galaxy Clusters , 2005, astro-ph/0504578.

[21]  Luc Simard,et al.  Spectroscopy of clusters in the ESO Distant Cluster Survey (EDisCS). Redshifts, velocity dispersions , 2004, astro-ph/0408071.

[22]  M. Nonino,et al.  K$_{\mbox{\fontsize{12pt}{14pt}\selectfont{\textit{s}}}}$-band luminosity function of the z = 1.237 cluster of galaxies RDCS J1252.9-2927 , 2004 .

[23]  Toulouse,et al.  The Buildup of the Red Sequence in Galaxy Clusters since z ∼ 0.8 , 2004, astro-ph/0406454.

[24]  G. Bruzual,et al.  Stellar population synthesis at the resolution of 2003 , 2003, astro-ph/0309134.

[25]  P. P. van der Werf,et al.  The Rest-Frame Optical Luminosity Density, Color, and Stellar Mass Density of the Universe from z = 0 to z = 3 , 2003, astro-ph/0307149.

[26]  G. Chabrier.  Galactic Stellar and Substellar Initial Mass Function , 2003, astro-ph/0304382.

[27]  Konrad Kuijken,et al.  A K-Band-selected Photometric Redshift Catalog in the Hubble Deep Field South: Sampling the Rest-Frame V Band to z = 3 , 2001, astro-ph/0106074.

[28]  A. Gonzalez,et al.  The Las Campanas Distant Cluster Survey: The Catalog , 2001, astro-ph/0106055.

[29]  R. Brunner,et al.  A Probabilistic Quantification of Galaxy Cluster Membership , 2000, astro-ph/0008462.

[30]  A. Kinney,et al.  The Dust Content and Opacity of Actively Star-forming Galaxies , 1999, astro-ph/9911459.

[31]  A. Pickles.  A Stellar Spectral Flux Library: 1150–25000 Å , 1998 .

[32]  D. Schlegel,et al.  Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .

[33]  D. Schlegel,et al.  Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds , 1997, astro-ph/9710327.

[34]  A. Kinney,et al.  Template ultraviolet to near-infrared spectra of star-forming galaxies and their application to K-corrections , 1996 .

[35]  E. Bertin,et al.  SExtractor: Software for source extraction , 1996 .

[36]  S. Charlot,et al.  Spectral evolution of stellar populations using isochrone synthesis , 1993 .

[37]  D. Weedman,et al.  Colors and magnitudes predicted for high redshift galaxies , 1980 .

[38]  A. Dressler.  Galaxy morphology in rich clusters: Implications for the formation and evolution of galaxies , 1980 .

[39]  Glenn E. Miller,et al.  The Initial mass function and stellar birthrate in the solar neighborhood , 1979 .

[40]  Y. Avni,et al.  Energy spectra of X-ray clusters of galaxies , 1976 .

[41]  C. Schlöder.  Online-Material , 2011, Tierärztliche Praxis G: Großtiere/Nutztiere.

[42]  E. Salpeter.  The Luminosity function and stellar evolution , 1955 .