activity
19932026
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 45k across the 393 of their papers we have counts for

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Showing 2008Show all

24 papers · 1 filter

astro-ph2008★ 110 cited

The Environments of Active Galactic Nuclei within the zCOSMOS Density Field

J. D. Silverman, K. Kovac, C. Knobel +58

The impact of environment on AGN activity up to z~1 is assessed by utilizing a mass-selected sample of galaxies from the 10k catalog of the zCOSMOS spectroscopic redshift survey. W…

astro-ph2008★ 107 cited

The spatial clustering of X-ray selected AGN in the XMM-COSMOS field

R. Gilli, G. Zamorani, T. Miyaji +70

We study the spatial clustering of 538 X-ray selected AGN in the 2 deg^2 XMM-COSMOS field that are spectroscopically identified to I_{AB}<23 and span the redshift range z=0.2-3.0.…

astro-ph2008★ 193 cited

Photometric redshifts for the CFHTLS T0004 Deep and Wide fields

J. Coupon, O. Ilbert, M. Kilbinger +15

We compute photometric redshifts based on the template-fitting method in the fourth public release of the Canada-France-Hawaii Telescope Legacy Survey. This unique multi-colour cat…

astro-ph2008★ 96 cited

Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. I. The evolution of the mass-metallicity relation up to z~0.9

F. Lamareille, J. Brinchmann, T. Contini +43

We derive the mass-metallicity relation of star-forming galaxies up to , using data from the VIMOS VLT Deep Survey. Automatic measurement of emission-line fluxes and equi…

astro-ph2008★ 10 cited

The VVDS-VLA Deep Field - IV: Radio-optical properties

S. Bardelli, E. Zucca, M. Bolzonella +51

(abridged) We use the 1.4 GHz VIMOS-VLA Deep Survey and the optical VVDS and the CFHT-LS to compare the properties of radio loud galaxies with respect to the whole population of op…

astro-ph2008★ 236 cited

Ongoing and co-evolving star formation in zCOSMOS galaxies hosting Active Galactic Nuclei

J. D. Silverman, F. Lamareille, C. Maier +60

We present a study of the host galaxies of AGN selected from the zCOSMOS survey to establish if accretion onto supermassive black holes and star formation are explicitly linked up…

astro-ph2008★ 57 cited

The zCOSMOS redshift survey: the three-dimensional classification cube and bimodality in galaxy physical properties

M. Mignoli, G. Zamorani, M. Scodeggio +56

Aims. We investigate the relationships between three main optical galaxy observables (spectral properties, colours, and morphology), exploiting the data set provided by the COSMOS/…

astro-ph2008★ 224 cited

Chasing highly obscured QSOs in the COSMOS field

F. Fiore, S. Puccetti, M. Brusa +41

(abridged) We take advantage of the deep Chandra and Spitzer coverage of a large area (more than 10 times the area covered by the Chandra deep fields, CDFs in the COSMOS field, to…

astro-ph2008★ 16 cited

The close environment of 24 micron galaxies at 0.6<z<1.0 in the COSMOS field

K. I. Caputi, K. Kovac, M. Bolzonella +62

We investigate the close environment of 203 Spitzer 24 micron-selected sources at 0.6<z<1.0 using zCOSMOS-bright redshifts and spectra of I<22.5 AB mag galaxies, over 1.5 sq. deg.…

astro-ph2008★ 105 cited

High redshift quasars in the COSMOS survey: the space density of z>3 X-ray selected QSOs

M. Brusa, A. Comastri, R. Gilli +19

We present a new measurement of the space density of high redshift (3.0<z<4.5), X-ray selected QSOs obtained by exploiting the deep and uniform multiwavelength coverage of the COSM…

astro-ph2008★ 380 cited

Photometric redshift and classification for the XMM-COSMOS sources

M. Salvato, G. Hasinger, O. Ilbert +40

We present photometric redshifts and spectral energy distribution (SED) classifications for a sample of 1542 optically identified sources detected with XMM in the COSMOS field. Our…

astro-ph2008★ 22 cited

The XMM-Newton survey of the ELAIS-S1 field II: optical identifications and multiwavelength catalogue of X-ray sources

C. Feruglio, F. Fiore, F. La Franca +13

We present optical identifications and a multi-band catalogue of a sample of 478 X-ray sources in the XMM and Chandra surveys of the central 0.6 deg^2 of the ELAIS-S1 field. The op…

astro-ph2008★ 187 cited

The VIMOS VLT Deep Survey :Evolution of the major merger rate since z~1 from spectroscopicaly confirmed galaxy pairs

L. de Ravel, O. Le Fèvre, L. Tresse +48

From the VIMOS VLT Deep Survey we use a sample of 6447 galaxies with I_{AB} < 24 to identify 251 pairs of galaxies, each member with a secure spectroscopic redshift, which are clos…

astro-ph2008★ 20 cited

The ESO-Spitzer Imaging extragalactic Survey (ESIS) II: VIMOS I,z wide field imaging of ELAIS-S1 and selection of distant massive galaxies

S. Berta, S. Rubele, A. Franceschini +13

(abridged) The ESIS survey is the optical follow up of the SWIRE/Spitzer in the ELAIS-S1 region of the sky. In the era of observational cosmology, the main efforts are focused on t…

astro-ph2008★ 162 cited

The Vimos VLT Deep Survey: Global properties of 20000 galaxies in the I_AB<=22.5 WIDE survey

B. Garilli, O. Le Fèvre, L. Guzzo +44

The VVDS-Wide survey has been designed with the general aim of tracing the large-scale distribution of galaxies at z~1 on comoving scales reaching ~100Mpc/h, while providing a good…

astro-ph2008★ 2 cited

A spectroscopic study of a z=1.6 galaxy overdensity with GMASS

Jaron Kurk, Andrea Cimatti, Gianni Zamorani +12

The Galaxy Mass Assembly ultra-deep Spectroscopic Survey samples a part of the CDFS to unprecedented depth. The resulting distribution of 150 z>1.4 redshifts reveals a significant…

astro-ph2008★ 131 cited

The VLA-COSMOS Survey: III. Further Catalog Analysis and the Radio Source Counts

M. Bondi, P. Ciliegi, E. Schinnerer +4

The VLA-COSMOS Large Project has imaged the 2 sq.deg. COSMOS field with a resolution of 1.5 arcsec and a sensitivity of about 11 microJy (1 sigma) yielding to a catalog of about 36…

astro-ph2008★ 78 cited

GMASS Ultradeep Spectroscopy of Galaxies at z~2. III: The emergence of the color bimodality at z~2

P. Cassata, A. Cimatti, J. Kurk +12

The aim of this work is to study the evolution of the rest frame color distribution of galaxies with the redshift, in particular in the critical interval 1.4<z<3. We combine ultrad…

astro-ph2008★ 149 cited

A new method to separate star forming from AGN galaxies at intermediate redshift: The submillijansky radio population in the VLA-COSMOS survey

V. Smolcic, E. Schinnerer, M. Scodeggio +21

We explore the properties of the submillijansky radio population at 20 cm by applying a newly developed optical color-based method to separate star forming (SF) from AGN galaxies a…

astro-ph2008★ 39 cited

The optical spectra of 24 micron galaxies in the COSMOS field: I. Spitzer/MIPS bright sources in the zCOSMOS-bright 10k catalogue

K. I. Caputi, S. J. Lilly, H. Aussel +23

We study zCOSMOS-bright optical spectra for 609 Spitzer/MIPS 24 micron-selected galaxies with S(24um)> 0.30 mJy and I<22.5 (AB mag) over 1.5 sq. deg. of the COSMOS field. From emis…

astro-ph2008★ 670 cited

A test of the nature of cosmic acceleration using galaxy redshift distortions

L. Guzzo, M. Pierleoni, B. Meneux +48

Observations of distant supernovae indicate that the Universe is now in a phase of accelerated expansion the physical cause of which is a mystery. Formally, this requires the inclu…

astro-ph2008★ 15 cited

The VIMOS VLT Deep Survey: Testing the gravitational instability paradigm at z ~ 1

C. Marinoni, L. Guzzo, A. Cappi +5

We have reconstructed the three-dimensional density fluctuation maps to z ~ 1.5 using the distribution of galaxies observed in the VVDS-Deep survey. We use this overdensity field t…

astro-ph2008★ 17 cited

The VIMOS VLT Deep Survey: The K-band follow-up in the 0226-04 field

S. Temporin, A. Iovino, M. Bolzonella +45

AIMS. We present a new Ks-band survey that represents a significant extension to the previous wide-field Ks-band imaging survey within the 0226-04 field of the VIMOS-VLT deep surve…

astro-ph2008★ 317 cited

GMASS Ultradeep Spectroscopy of Galaxies at 1.4<z<2. II. Superdense passive galaxies: how did they form and evolve ?

A. Cimatti, P. Cassata, L. Pozzetti +13

We combine ultradeep optical spectroscopy from the GMASS project ("Galaxy Mass Assembly ultradeep Spectroscopic Survey") with GOODS multi-band photometry and HST imaging to study a…