论文信息 - Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey - 字舞流文

Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey

We present photometric redshifts for an uniquely large and deep sample of 522286 objects with i'_{AB}<25 in the Canada-France Legacy Survey ``Deep Survey'' fields, which cover a total effective area of 3.2 deg^2. We use 3241 spectroscopic redshifts with 0

B. Garilli | L. Guzzo | Y. Mellier | R. Scaramella | O. Fèvre | S. Paltani | G. Zamorani | M. Scodeggio | S. Bardelli | P. Franzetti | O. Ilbert | H. McCracken | R. Pelló | L. Pozzetti | M. Radovich | S. Arnouts | E. Bertin | G. Vettolani | S. L. Torre | V. Ripepi | S. Foucaud | A. Zanichelli | D. Rizzo | M. Bolzonella | C. Adami | D. Bottini | A. Cappi | O. Cucciati | A. Iovino | V. Brun | D. Maccagni | A. Pollo | D. Vergani | C. Marinoni | A. Bongiorno | A. Mazure | E. Zucca | B. Marano | S. Charlot | T. Contini | L. Tresse | J. Picat | I. Gavignaud | G. Mathez | B. Meneux | R. Merighi | M. Bondi | A. Bongiorno | G. Busarello | P. Ciliegi | P. Merluzzi | F. Lamareille | L. Gregorini | S. D. Torre

[1] L. Moscardini,et al. Measuring the Redshift Evolution of Clustering: the Hubble Deep Field South , 2002 .

[2] A. Cimatti,et al. A catalogue of the Chandra Deep Field South with multi-colour classification and photometric redshifts from COMBO-17 , 2004, astro-ph/0403666.

[3] Oxford,et al. The COMBO-17 survey: Evolution of the galaxy luminosity function from 25,000 galaxies with 0.2 < z < 1.2 , 2002, astro-ph/0208345.

[4] Stephan Aune,et al. MegaCam: the new Canada-France-Hawaii Telescope wide-field imaging camera , 2003, SPIE Astronomical Telescopes + Instrumentation.

[5] A. Fontana,et al. Photometric Redshifts and Selection of High-Redshift Galaxies in the NTT and Hubble Deep Fields , 2000, astro-ph/0009158.

[6] A. Fontana,et al. Photometric redshifts with the Multilayer Perceptron Neural Network: Application to the HDF-S and SDSS , 2003, astro-ph/0312064.

[7] A. Mazure,et al. The VIMOS VLT deep survey , 2008, 0903.0271.

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

[9] M. Dickinson,et al. Photometric Redshifts for Galaxies in the GOODS Southern Field , 2003, astro-ph/0309068.

[10] 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.

[11] H. Lin,et al. Evolution of the Galaxy Population Based on Photometric Redshifts in the Hubble Deep Field , 1997 .

[12] Oliver LeFevre,et al. Commissioning and performances of the VLT-VIMOS , 2003, SPIE Astronomical Telescopes + Instrumentation.

[13] I. Tereno,et al. Cosmic shear analysis with CFHTLS deep data , 2005, astro-ph/0511090.

[14] A. Mazure,et al. A large population of galaxies 9 to 12 billion years back in the history of the Universe , 2005, Nature.

[15] R. Bouwens,et al. Faint Galaxies in Deep Advanced Camera for Surveys Observations , 2004 .

[16] Edwin L. Turner,et al. A Catalog of Color-based Redshift Estimates for Z <~ 4 Galaxies in the Hubble Deep Field , 1998 .

[17] Andrew J. Connolly,et al. Creating Spectral Templates from Multicolor Redshift Surveys , 1999, astro-ph/9908008.

[18] M. Dantel-Fort,et al. The VIRMOS deep imaging survey: II: CFH12K BVRI optical data for the 0226-04 deep field , 2003 .

[19] S. Noll,et al. The evolution of the luminosity functions in the FORS Deep Field from low to high redshift: I. The blue bands , 2004, astro-ph/0403535.

[20] R. Kron. Photometry of a complete sample of faint galaxies. , 1980 .

[21] Jonathan P. Gardner,et al. The Redshift Distribution of Near-Infrared-selected Galaxies in the Great Observatories Origins Deep Survey as a Test of Galaxy Formation Scenarios , 2003, astro-ph/0309067.

[22] A. Szalay,et al. Slicing Through Multicolor Space: Galaxy Redshifts from Broadband Photometry , 1995, astro-ph/9508100.

[23] B. Garilli,et al. The VIRMOS deep imaging survey IV: Near-infrared observations , 2005, astro-ph/0507668.

[24] L. Moscardini,et al. Measuring and modelling the redshift evolution of clustering: the Hubble Deep Field North , 1999, astro-ph/9902290.

[25] Frazer N. Owen,et al. Near-infrared photometry of distant radio galaxies - Spectral flux distributions and redshift estimates , 1982 .

[26] A. Cimatti,et al. The K20 survey - IV. The redshift distribution of $K_{\rm s}<20$ galaxies: A test of galaxy formation models , 2002, astro-ph/0207191.

[27] Piero Madau,et al. Radiative transfer in a clumpy universe: The colors of high-redshift galaxies , 1995 .

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

[29] A. Mazure,et al. The VIMOS-VLT deep survey - Evolution of the galaxy luminosity function up to z = 2 in first epoch data , 2004, astro-ph/0409134.

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

[31] N. Benı́tez. Bayesian Photometric Redshift Estimation , 1998, astro-ph/9811189.

[32] France,et al. Luminosity functions beyond the spectroscopic limit I. Method and near-infrared LFs in the HDF-N and HDF-S , 2002 .

[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. Mazure,et al. The VIRMOS deep imaging survey: I. overview and survey strategy , 2002 .

[35] A. Fernandez-Soto,et al. A New Catalog of Photometric Redshifts in the Hubble Deep Field , 1999 .

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

[37] S. J. Lilly,et al. The Canada-France Deep Fields Survey. III. Photometric Redshift Distribution to IAB = 24 , 2003, astro-ph/0310038.

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

[39] A. J. Connolly,et al. Reconstructing Galaxy Spectral Energy Distributions from Broadband Photometry , 1999, astro-ph/9910389.

[40] Guinevere Kauffmann,et al. The K-band luminosity function at z = 1: a powerful constraint on galaxy formation theory , 1998 .

[41] N. Vogt,et al. The Nature of Compact Galaxies in the Hubble Deep Field. I. Global Properties , 1997 .

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