The VIMOS VLT Deep Survey: the group catalogue (2009)
Cucciati, O., Marinoni, C., Iovino, A., Bardelli, S., Adami, C., Mazure, A., ...
[Abridged] We used the purely flux limited (17.5
The [OIII] emission line luminosity function of optically selected type-2 AGN from zCOSMOS (2009)
Bongiorno, A., Mignoli, M., Zamorani, G., Lamareille, F., Lanzuisi, G., Miyaji, T., ...
We present a catalog of 213 type-2 AGN selected from the zCOSMOS survey. The selected sample covers a wide redshift range (0.15
Properties and environment of Radio Emitting Galaxies in the VLA-zCOSMOS survey (2009)
Bardelli, S., Schinnerer, E., Smolcic, V., Zamorani, G., Zucca, E., Mignoli, M., ...
We investigate the properties and the environment of radio sources with optical counterpart from the combined VLA-COSMOS and zCOSMOS samples. The advantage of this sample is the availability of...
Orsi, Alvaro, Baugh, C. M., Lacey, C. G., Cimatti, A., Wang, Y., Zamorani, G.
Future galaxy surveys will map the galaxy distribution in the redshift interval $0.5
Empirical H-alpha emitter count predictions for dark energy surveys (2009)
Geach, J. E., Cimatti, A., Percival, W., Wang, Y., Guzzo, L., Zamorani, G., ...
Future galaxy redshift surveys aim to measure cosmological quantities from the galaxy power spectrum. A prime example is the detection of baryonic acoustic oscillations (BAOs), providing a standard...
Caputi, K. I., Lilly, S. J., Aussel, H., Floc'h, E. Le, Sanders, D., Maier, C., ...
We have used the zCOSMOS-bright 10k sample to identify 3244 Spitzer/MIPS 24-micron-selected galaxies with 0.06< S(24um)< 0.50 mJy and I(AB)
Rodighiero, G., Vaccari, M., Franceschini, A., Tresse, L., Fevre, O. Le, Brun, V. Le, ...
[Abridged]We exploit a large homogeneous dataset to derive a self-consistent picture of IR emission based on the time-dependent 24, 15, 12 and 8micron monochromatic and bolometric IR luminosity...
Merloni, A., Bongiorno, A., Bolzonella, M., Brusa, M., Civano, F., Comastri, A., ...
(Abriged) We report on the measurement of the rest frame K-band luminosity and total stellar mass of the hosts of 89 broad line Active Galactic Nuclei detected in the zCOSMOS survey in the redshift...
The Chandra survey of the COSMOS field II: source detection and photometry (2009)
Puccetti, S., Vignali, C., Cappelluti, N., Fiore, F., Zamorani, G., Aldcroft, T. L., ...
The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra program, that covers the central contiguous ~0.92 deg^2 of the COSMOS field. C-COSMOS is the result of a complex tiling, with every...
Black Hole Growth and Starburst Activity at z=0.6-4 in the Chandra Deep Field South (2009)
Brusa, M., Fiore, F., Santini, P., Grazian, A., Comastri, A., Zamorani, G., ...
The co-evolution of host galaxies and the active black holes which reside in their centre is one of the most important topics in modern observational cosmology. Here we present a study of the...
The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1 (2009)
Kovac, K., Porciani, C., Lilly, S. J., Marinoni, C., Guzzo, L., Cucciati, O., ...
We use the overdensity field reconstructed in the volume of the COSMOS area to study the nonlinear biasing of the zCOSMOS galaxies. The galaxy overdensity field is reconstructed using the current...
Sacchi, N., La Franca, F., Feruglio, C., Fiore, F., Puccetti, S., Cocchia, F., ...
We present a catalog of optical spectroscopic identifications of sources detected by Spitzer at 3.6 or 24 μm down to ~10 and ~280 μJy, respectively, in the SWIRE/XMM-Newton/ELAIS-S1 field and...
Zucca, E., Bardelli, S., Bolzonella, M., Zamorani, G., Ilbert, O., Pozzetti, L., ...
(Abridged) We studied the evolution in the B band luminosity function to z~1 in the zCOSMOS 10k sample, for which both accurate galaxy classifications and a detailed description of the local density...
Sacchi, N., La Franca, F., Feruglio, C., Fiore, F., Puccetti, S., Cocchia, F., ...
We present a catalog of optical spectroscopic identifications of sources detected by Spitzer at 3.6 or 24 micron down to 10 and 280 microJy, respectively, in the SWIRE/XMM-Newton/ELAIS-S1 field and...
The 10k zCOSMOS: morphological transformation of galaxies in the group environment since z~1 (2009)
Kovac, K., Lilly, S. J., Knobel, C., Bolzonella, M., Iovino, A., Carollo, C. M., ...
We study the evolution of galaxies inside and outside of the group environment since z=1 using a large well defined set of groups and galaxies from the zCOSMOS-bright redshift survey in the COSMOS...
The zCOSMOS Redshift Survey: How group environment alters global downsizing trends (2009)
Iovino, A., Cucciati, O., Scodeggio, M., Knobel, C., Kovac, K., Lilly, S., ...
We took advantage of the wealth of information provided by the first ~10000 galaxies of the zCOSMOS-bright survey and its group catalogue to study the complex interplay between group environment and...
Vergani, D., Zamorani, G., Lilly, S. J., Lamareille, F., Halliday, C., Scodeggio, M., ...
The identities of the main processes triggering and quenching star-formation in galaxies remain unclear. A key stage in evolution, however, appears to be represented by post-starburst galaxies. To...
The Chandra COSMOS Survey. I. Overview and Point Source Catalog (2009)
Elvis, Martin, Civano, Francesca, Vignali, Cristian, Puccetti, Simonetta, Fiore, Fabrizio, Cappelluti, Nico, ...
The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra program that has imaged the central 0.5 deg^2 of the COSMOS field (centered at 10 ^h , +02 ^o ) with an effective exposure of ~160 ks,...
Pozzetti, L., Bolzonella, M., Zucca, E., Zamorani, G., Lilly, S., Renzini, A., ...
We present the Galaxy Stellar Mass Function (GSMF) up to z~1 from the zCOSMOS-bright 10k spectroscopic sample. We investigate the total MF and the contribution of ETGs and LTGs, defined by broad-band...
Bolzonella, M., Kovac, K., Pozzetti, L., Zucca, E., Cucciati, O., Lilly, S. J., ...
We study the impact of the environment on the evolution of galaxies in the zCOSMOS 10k sample in the redshift range 0.1
Kurk, J., Cimatti, A., Zamorani, G., Halliday, C., Mignoli, M., Pozzetti, L., ...
We present a study of a galaxy overdensity at z=1.6, Cl 0332-2742, uncovered in the Galaxy Mass Assembly ultra-deep Spectroscopic Survey (GMASS). We conservatively estimate the overdensity in...
Tasca, L. A. M., Kneib, J. P., Iovino, A., Fevre, O. Le, Kovac, K., Bolzonella, M., ...
For more than two decades we have known that galaxy morphological segregation is present in the Local Universe. It is important to see how this relation evolves with cosmic time. To investigate how...
Dynamical masses of early-type galaxies at z~2: Are they truly superdense? (2009)
Cappellari, Michele, Alighieri, S. Di Serego, Cimatti, A., Daddi, E., Renzini, A., Kurk, J. D., ...
We measured stellar velocity dispersions sigma and dynamical masses of 9 massive (M~10^11 Msun) early-type galaxies (ETG) from the GMASS sample at redshift 1.4
The zCOSMOS Survey. The dependence of clustering on luminosity and stellar mass at z=0.2-1 (2009)
Meneux, B., Guzzo, L., Porciani, C., Zamorani, G., Abbas, U., ...
We study the dependence of galaxy clustering on luminosity and stellar mass at redshifts z ~ [0.2-1] using the first zCOSMOS 10K sample. We measure the redshift-space correlation functions xi(rp,pi)...
Cosmic Evolution of Radio Selected Active Galactic Nuclei in the Cosmos Field (2009)
Smolčić, V., Zamorani, G., Schinnerer, E., Bardelli, S., Bondi, M., Bîrzan, L., ...
We explore the cosmic evolution of radio luminous active galactic nuclei (AGNs) with low radio powers (L_(1.4 GHz) ≾ 5 × 10^(25) W Hz^(–1)) out to z = 1.3 using to date the largest sample of...
Ongoing and Co-Evolving Star Formation in zCOSMOS Galaxies Hosting Active Galactic Nuclei (2009)
Silverman, J. D., Lamareille, F., Maier, C., Lilly, S. J., Mainieri, V., Brusa, M., ...
We present a study of the host galaxies of active galactic nucleus (AGN) selected from the zCOSMOS survey to establish if accretion onto supermassive black holes (SMBHs) and star formation are...
The Environments of Active Galactic Nuclei within the zCOSMOS Density Field (2009)
Silverman, J. D., Kovač, K., Knobel, C., Lilly, S., Bolzonella, M., Lamareille, F., ...
The impact of environment on active galactic nucleus (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...
Maier, C., Lilly, S. J., Zamorani, G., Scodeggio, M., Lamareille, F., Contini, T., ...
In order to try to understand the internal evolution of galaxies and relate this to the global evolution of the galaxy population, we present a comparative study of the dependence of star formation...
GMASS ultradeep spectroscopy of galaxies at z ~ 2. IV. The variety of dust populations (2009)
Noll, S., Pierini, D., Cimatti, A., Daddi, E., Kurk, J. D., Bolzonella, M., ...
The properties of dust attenuation at rest-frame UV wavelengths are inferred from very high-quality FORS2 spectra of 78 galaxies from the GMASS survey at 1
The density field of the 10k zCOSMOS galaxies (2009)
Kovac, K., Lilly, S. J., Cucciati, O., Porciani, C., Iovino, A., Zamorani, G., ...
We use the current sample of ~10,000 zCOSMOS spectra of sources selected with I(AB) < 22.5 to define the density field out to z~1, with much greater resolution in the radial dimension than has been...
An optical group catalogue to z = 1 from the zCOSMOS 10k sample (2009)
Knobel, C., Lilly, S. J., Iovino, A., Porciani, C., Kovac, K., Cucciati, O., ...
We present a galaxy group catalogue spanning the redshift range 0.1
The Chandra COSMOS Survey, I: Overview and Point Source Catalog (2009)
Elvis, Martin, Civano, Francesca, Vignali, Cristian, Puccetti, Simonetta, Fiore, Fabrizio, Cappelluti, Nico, ...
The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra} program that has imaged the central 0.5 sq.deg of the COSMOS field (centered at 10h, +02deg) with an effective exposure of ~160ksec,...
Scodeggio, M., Vergani, D., Cucciati, O., Iovino, A., Franzetti, P., Garilli, B., ...
Hierarchical models of galaxy formation predict that the properties of a dark matter halo depend on the large-scale environment surrounding the halo. As a result of this correlation, we expect...
High-redshift quasars in the cosmos survey: the space density of z > 3 x-ray selected QSOs (2009)
Brusa, M., Comastri, A., Gilli, R., Hasinger, G., Iwasawa, K., Mainieri, V., ...
We present a new measurement of the space density of high-redshift (z ≃ 3.0-4.5), X-ray-selected quasi-stellar objects (QSOs) obtained by exploiting the deep and uniform multiwavelength coverage of...
Chasing highly obscured QSOs in the cosmos field (2009)
Fiore, F., Puccetti, S., Brusa, M., Salvato, M., Zamorani, G., Aldcroft, T., ...
A large population of heavily obscured, Compton-thick active galactic nuclei (AGNs) is predicted by AGN synthesis models for the cosmic X-ray background and by the "relic" supermassive black hole...
SPACE: the spectroscopic all-sky cosmic explorer (2009)
Cimatti, A., Robberto, M., Baugh, C., Beckwith, S. V. W., Content, R., Daddi, E., ...
We describe the scientific motivations, the mission concept and the instrumentation of SPACE, a class-M mission proposed for concept study at the first call of the ESA Cosmic-Vision 2015–2025...
Galaxy Stellar Mass Assembly between 0.2 (2009)
Ilbert, O., Salvato, M., Floc'h, E. Le, Aussel, H., Capak, P., McCracken, H. J., ...
We follow the galaxy stellar mass assembly by morphological and spectral type in the COSMOS 2-deg^2 field. We derive the stellar mass functions and stellar mass densities from z=2 to z=0.2 using...
Vignali, C., Pozzi, F., Fritz, J., Comastri, A., Gruppioni, C., Bellocchi, E., ...
We present multi-wavelength observations (from optical to sub-millimeter, including Spitzer and SCUBA) of H2XMMJ 003357.2-120038 (also GD158_19), an X-ray selected, luminous narrow-line (Type 2)...
The XMM-Newton wide-field survey in the COSMOS field - The point-like X-ray source catalogue (2009)
Cappelluti, N., Brusa, M., Hasinger, G., Comastri, A., Zamorani, G., Finoguenov, A., ...
Context. The COSMOS survey is a multiwavelength survey aimed to study the evolution of galaxies, AGN and large scale structures. Within this survey XMM-COSMOS a powerful tool to detect AGN and galaxy...
Vignali, C., Fiore, F., Comastri, A., Brusa, M., Gilli, R., Cappelluti, N., ...
Here we review some of the main issues related to multi-wavelength source identification and characterization, with particular emphasis on the field of X-ray surveys carried out over the last years....
Cosmic evolution of radio selected active galactic nuclei in the COSMOS field (2009)
Smolcic, V., Zamorani, G., Schinnerer, E., Bardelli, S., Bondi, M., Birzan, L., ...
We explore the cosmic evolution of radio AGN with low radio powers (L_1.4GHz < 5\times10^25 W/Hz) out to z=1.3 using to-date the largest sample of ~600 low luminosity radio AGN at intermediate...
The close environment of 24 μm galaxies at 0.6 < z < 1.0 in the cosmos field (2009)
Caputi, K. I., Kovač, K., Bolzonella, M., Lilly, S. J., Zamorani, G., Aussel, H., ...
We investigate the close environment of 203 Spitzer 24 μm -selected sources at 0.6 < z < 1.0 using zCOSMOS-bright redshifts and spectra of I < 22.5 AB mag galaxies, over 1.5 deg^2 of the COSMOS...
The XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogue (2009)
Cappelluti, N., Brusa, M., Hasinger, G., Comastri, A., Zamorani, G., Finoguenov, A., ...
The COSMOS survey is a multiwavelength survey aimed to study the evolution of galaxies, AGN and the large scale structure. The XMM-COSMOS is a deep X-ray survey over the full 2 deg2 of the COSMOS...
Photometric Redshift and Classification for the XMM-COSMOS Sources (2009)
Salvato, M., Hasinger, G., Ilbert, O., Zamorani, G., Brusa, M., Scoville, N. Z., ...
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 template fitting...
Cosmos Photometric Redshifts with 30-Bands for 2-deg^2 (2009)
Ilbert, O., Capak, P., Salvato, M., Aussel, H., McCracken, H. J., Sanders, D. B., ...
We present accurate photometric redshifts (photo-z) in the 2-deg^2 COSMOS field. The redshifts are computed with 30 broad, intermediate, and narrowbands covering the UV (Galaxy Evolution Explorer),...
The Evolution of the Star Formation of zCOSMOS and SDSS galaxies at z (2009)
Maier, C., Lilly, S. J., Zamorani, G., Scodeggio, M., Lamareille, F., Contini, T., ...
We present in these proceedings some preliminary results we have obtained studying the evolution of the specific star formation rate as a function of surface mass density and Sersic indices at z
Maier, C., Lilly, S. J., Zamorani, G., Scodeggio, M., Lamareille, F., Contini, T., ...
In order to try to understand the internal evolution of galaxies and relate this to the global evolution of the galaxy population, we present a comparative study of the dependence of star formation...
The Dust-Unbiased Cosmic Star-Formation History from the 20 CM VLA-COSMOS Survey (2009)
Smolčić, V., Schinnerer, E., Zamorani, G., Bell, E. F., Bondi, M., Carilli, C. L., ...
We derive the cosmic star-formation history out to z = 1.3 using a sample of ~350 radio-selected star-forming (SF) galaxies, a far larger sample than those in previous, similar studies. We attempt to...
Mignoli, M., Zamorani, G., Scodeggio, M., Cimatti, A., Halliday, C., Lilly, S. J., ...
Aims. We investigate the relationships between three main optical galaxy observables (spectral properties, colors, and morphology), exploiting the data set provided by the COSMOS/zCOSMOS survey. The...
Mignoli, M., Zamorani, G., Scodeggio, M., Cimatti, A., Halliday, C., Lilly, S. J., ...
Aims. We investigate the relationships between three main optical galaxy observables (spectral properties, colors, and morphology), exploiting the data set provided by the COSMOS/zCOSMOS survey. The...
The spatial clustering of X-ray selected AGN in the XMM-COSMOS field (2009)
Gilli, R., Zamorani, G., Miyaji, T., Silverman, J., Brusa, M., Mainieri, V., ...
We study the spatial clustering of 538 X-ray selected AGN in the 2 deg^2 XMM-COSMOS field that are spectroscopically identified with I_(AB) < 23 and span the redshift range z = 0.2−3.0. The median...
Lamareille, F., Brinchmann, J., Contini, T., Walcher, C.J., Charlot, S., Pérez-Montero, E., ...
We derive the mass-metallicity relation of star-forming galaxies up to $z\sim0.9$, using data from the VIMOS VLT Deep Survey. Automatic measurement of emission-line fluxes and equivalent widths have...
Lamareille, F., Brinchmann, J., Contini, T., Walcher, C.J., Charlot, S., Pérez-Montero, E., ...
We derive the mass-metallicity relation of star-forming galaxies up to $z\sim0.9$, using data from the VIMOS VLT Deep Survey. Automatic measurement of emission-line fluxes and equivalent widths have...
Photometric redshift and classification for the XMM-COSMOS sources (2009)
Salvato, M., Hasinger, G., Ilbert, O., Zamorani, G., Brusa, M., Scoville, N. Z., ...
Cosmos photometric redshifts with 30-bands for 2-deg2 (2009)
Ilbert, O., Capak, P., Salvato, M., Aussel, H., McCracken, H. J., Sanders, D. B., ...
The spatial clustering of X-ray selected AGN in the XMM-COSMOS field (2009)
Gilli, R., Zamorani, G., Miyaji, T., Silverman, J., Brusa, M., Mainieri, V., ...
The close environment of 24 μm galaxies at 0.6 < z < 1.0 in the cosmos field (2009)
Caputi, K. I., Kovac, K., Bolzonella, M., Lilly, S. J., Zamorani, G., Aussel, H., ...
The VVDS-VLA deep field - IV. Radio-optical properties (2009)
Bardelli, S., Zucca, E., Bolzonella, M., Ciliegi, P., Gregorini, L., Zamorani, G., ...
Chasing highly obscured QSOs in the COSMOS field (2009)
Fiore, F., Puccetti, S., Brusa, M., Salvato, M., Zamorani, G., Aldcroft, T., ...
High-redshift quasars in the COSMOS survey: the space density of z > 3 X-ray selected QSOs (2009)
Brusa, M., Comastri, A., Gilli, R., Hasinger, G., Iwasawa, K., Mainieri, V., ...
An optical group catalog to z = 1 from the zCOSMOS 10 k sample (2009)
Knobel, C., Lilly, S. J., Iovino, A., Porciani, C., Kovac, K., Cucciati, O., ...
The XMM-Newton wide-field survey in the COSMOS field The point-like X-ray source catalogue (2009)
Cappelluti, N., Brusa, M., Hasinger, G., Comastri, A., Zamorani, G., Finoguenov, A., ...
Cosmic evolution of radio selected active galactic nuclei in the cosmos field (2009)
Smolcic, V., Zamorani, G., Schinnerer, E., Bardelli, S., Bondi, M., Birzan, L., ...
GMASS ultradeep spectroscopy of galaxies at z ~ 2 - IV. The variety of dust populations (2009)
Noll, S., Pierini, D., Cimatti, A., Daddi, E., Kurk, J. D., Bolzonella, M., ...
The Chandra COSMOS Survey. I. Overview and Point Source Catalog (2009)
Elvis, M., Civano, F., Vignali, C., Puccetti, S., Fiore, F., Cappelluti, N., ...
The Chandra COSMOS survey - I. Overview and point source catalog (2009)
Elvis, Martin, Civano, Francesca, Vignali, Christian, Puccetti, Simonetta, Fiore, Fabrizio, Cappelluti, Nico, ...
The Environments of Active Galactic Nuclei within the zCOSMOS Density Field (2008)
Silverman, J. D., Kovac, K., Knobel, C., Lilly, S., Bolzonella, M., Lamareille, F., ...
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. We identify 147 AGN...
Walcher, C. J., Lamareille, F., Vergani, D., Arnouts, S., Buat, V., Charlot, S., ...
Measuring the build-up of stellar mass is one of the main objectives of studies of galaxy evolution. Traditionally, the mass in stars and the star formation rates have been measured by different...
Photometric redshifts for the CFHTLS T0004 Deep and Wide fields (2008)
Coupon, J., Ilbert, O., Kilbinger, M., McCracken, H. J., Mellier, Y., Arnouts, S., ...
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 catalogue comprises...
Testing gravity on large scales. The skewness of the galaxy distribution at z~1 (2008)
Marinoni, C., Guzzo, L., Cappi, A., Fevre, O. Le, Mazure, A., Meneux, B., ...
We study the evolution of the low-order moments of the galaxy overdensity distribution over the redshift interval 0.7
Lamareille, F., Brinchmann, J., Contini, T., Walcher, C. J., Charlot, S., Pérez-Montero, E., ...
We derive the mass-metallicity relation of star-forming galaxies up to $z\sim0.9$, using data from the VIMOS VLT Deep Survey. Automatic measurement of emission-line fluxes and equivalent widths have...
Perez-Montero, E., Contini, T., Lamareille, F., Brinchmann, J., Walcher, C. J., Charlot, S., ...
Aims. We present a continuation of our study about the relation between stellar mass and gas-phase metallicity in the VIMOS VLT Deep Survey (VVDS). In this work we extend the determination of...
The VVDS-VLA Deep Field - IV: Radio-optical properties (2008)
Bardelli, S., Zucca, E., Bolzonella, M., Ciliegi, P., Gregorini, L., Zamorani, G., ...
(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 optical galaxies. The...
The spatial clustering of X-ray selected AGN in the XMM-COSMOS field (2008)
Gilli, R., Zamorani, G., Miyaji, T., Silverman, J., Brusa, M., Mainieri, V., ...
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} 3 x 10^{10} M_sun) at the same redshift. This suggests that...
Ongoing and co-evolving star formation in zCOSMOS galaxies hosting Active Galactic Nuclei (2008)
Silverman, J. D., Lamareille, F., Maier, C., Lilly, S., Mainieri, V., Brusa, M., ...
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 to z~1. We identify...
Gavignaud, I., Wisotzki, L., Bongiorno, A., Paltani, S., Zamorani, G., Møller, P., ...
We use one of the deepest spectroscopic samples of broad line active galactic nuclei (AGN) currently available, extracted from the VIMOS VLT Deep Survey (VVDS), to compute MgII and CIV virial masses...
Mignoli, M., Zamorani, G., Scodeggio, M., Cimatti, A., Halliday, C., Lilly, S. J., ...
Aims. We investigate the relationships between three main optical galaxy observables (spectral properties, colours, and morphology), exploiting the data set provided by the COSMOS/zCOSMOS survey. The...
Chasing highly obscured QSOs in the COSMOS field (2008)
Fiore, F., Puccetti, S., Brusa, M., Salvato, M., Zamorani, G., Aldcroft, T., ...
(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 extend the search...
High redshift quasars in the COSMOS survey: the space density of z>3 X-ray selected QSOs (2008)
Brusa, M., Comastri, A., Gilli, R., Hasinger, G., Iwasawa, K., Mainieri, V., ...
We present a new measurement of the space density of high redshift (3.03 QSOs for which spectroscopic (22) or photometric (18) redshifts are available. We present the optical (color-color diagrams)...
Photometric redshift and classification for the XMM-COSMOS sources (2008)
Salvato, M., Hasinger, G., Ilbert, O., Zamorani, G., Brusa, M., Scoville, N., ...
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 template fitting...
COSMOS Photometric Redshifts with 30-bands for 2-deg2 (2008)
Ilbert, O., Capak, P., Salvato, M., Aussel, H., McCracken, H. J., Sanders, D. B., ...
We present accurate photometric redshifts in the 2-deg2 COSMOS field. The redshifts are computed with 30 broad, intermediate, and narrow bands covering the UV (GALEX), Visible-NIR (Subaru, CFHT,...
Gruppioni, C., Pozzi, F., Polletta, M., Zamorani, G., La Franca, F., Sacchi, N., ...
We present the broadband SEDs of the largest available highly complete (72%) spectroscopic sample of MIR-selected galaxies and AGNs at intermediate redshift. The sample contains 203 extragalactic...
Berta, S., Rubele, S., Franceschini, A., Held, E. V., Rizzi, L., Rodighiero, G., ...
Context. The ESO-Spitzer Imaging extragalactic Survey (ESIS) is the optical follow up of the Spitzer Wide-area Infra-Red Extragalactic survey (SWIRE) in the ELAIS-S1 region of the sky. Aims. In the...
The close environment of 24 micron galaxies at 0.6 (2008)
Caputi, K. I., Kovac, K., Bolzonella, M., Lilly, S. J., Zamorani, G., Aussel, H., ...
We investigate the close environment of 203 Spitzer 24 micron-selected sources at 0.6
The dust un-biased cosmic star formation history from the 20 cm VLA-COSMOS survey (2008)
Smolcic, V., Schinnerer, E., Zamorani, G., Bell, E. F., Bondi, M., Carilli, C. L., ...
We derive the cosmic star formation history (CSFH) out to z=1.3 using a sample of ~350 radio-selected star-forming galaxies, a far larger sample than in previous, similar studies. We attempt to...
Walcher, C. J., Lamareille, F., Vergani, D., Arnouts, S., Buat, V., Charlot, S., ...
We intend to show that it is possible to derive the physical parameters of galaxies from their broad-band spectral energy distribution out to a redshift of 1.2. This method has the potential to yield...
De Ravel, L., Fèvre, O. Le, Tresse, L., Bottini, D., Garilli, B., Brun, V. Le, ...
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 close in both projected...
Berta, S., Rubele, S., Franceschini, A., Held, E., Rizzi, L., Rodighiero, G., ...
(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 the study of galaxy...
Smolčić, V., Schinnerer, E., Scodeggio, M., Franzetti, P., Aussel, H., Bondi, M., ...
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 active galactic nucleus (AGN)...
Feruglio, C., Fiore, F., La Franca, F., Sacchi, N., Puccetti, S., Comastri, A., ...
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 optical/infrared...
Caputi, K. I., Lilly, S. J., Aussel, H., Sanders, D., Frayer, D., Le Févre, O., ...
We study zCOSMOS-bright optical spectra for 609 Spitzer MIPS 24 μm-selected galaxies with S_(24) μ m > 0.30 mJy and I < 22.5 (AB mag) over 1.5 deg^2 of the COSMOS field. From emission-line...
Gruppioni, C., Pozzi, F., Polletta, M., Zamorani, G., La Franca, F., Sacchi, N., ...
We present the broad-band Spectral Energy Distributions (SEDs) of the largest available highly (72%) complete spectroscopic sample of mid-infrared (MIR) selected galaxies and AGN at intermediate...
The Vimos VLT Deep Survey: Global properties of 20000 galaxies in the I_AB (2008)
Garilli, B., Fèvre, O. Le, Guzzo, L., Maccagni, D., Brun, V. Le, ...
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 control of cosmic...
The VLA-COSMOS Survey: III. Further Catalog Analysis and the Radio Source Counts (2008)
Bondi, M., Ciliegi, P., Schinnerer, E., Smolcic, V., Jahnke, K., Carilli, C., ...
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 3600 radio sources....
Cassata, P., Cimatti, A., Kurk, J., Rodighiero, G., Pozzetti, L., Bolzonella, M., ...
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 1.42 are passively evolving, with the bulk of...
Smolcic, V., Schinnerer, E., Scodeggio, M., Franzetti, P., Aussel, H., Bondi, M., ...
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 at intermediate...
Caputi, K. I., Lilly, S. J., Aussel, H., Sanders, D., Frayer, D., Fevre, O. Le, ...
We study zCOSMOS-bright optical spectra for 609 Spitzer/MIPS 24 micron-selected galaxies with S(24um)> 0.30 mJy and I
A test of the nature of cosmic acceleration using galaxy redshift distortions (2008)
Guzzo, L., Pierleoni, M., Meneux, B., Branchini, E., Fevre, O. Le, Marinoni, C., ...
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 inclusion of a term...
The VIMOS VLT Deep Survey: The K-band follow-up in the 0226-04 field (2008)
Temporin, S., Iovino, A., Bolzonella, M., McCracken, H. J., Scodeggio, M., Garilli, B., ...
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 survey (VVDS). The new...
GMASS Ultradeep Spectroscopy of Galaxies at 1.4 (2008)
Cimatti, A., Cassata, P., Pozzetti, L., Kurk, J., Mignoli, M., Renzini, A., ...
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 sample of passive...
GMASS Ultradeep Spectroscopy of Galaxies at redshift z~2. I. The stellar metallicity (2008)
Halliday, C., Daddi, E., Cimatti, A., Kurk, J., Renzini, A., Mignoli, M., ...
Context: Galaxy metallicities have been measured to redshift z~2 by gas-phase oxygen abundances of the interstellar medium using the R23 and N2 methods. Galaxy stellar metallicities provide crucial...
A test of the nature of cosmic acceleration using galaxy redshift distortions (2008)
Guzzo, L., Pierleoni, M., Meneux, B., Branchini, E., Le Fèvre, O., Marinoni, C., ...
A test of the nature of cosmic acceleration using galaxy redshift distortions (2008)
Guzzo, L., Pierleoni, M., Meneux, B., Branchini, E., Le Fèvre, O., Marinoni, C., ...
Unveiling obscured accretion in the Chandra deep field–south (2008)
Fiore, F., Grazian, A., Santini, P., Puccetti, S., Brusa, M., Feruglio, C., ...
The VIMOS VLT deep survey: testing the gravitational instability paradigm at z ~ 1 (2008)
Marinoni, C., Guzzo, L., Cappi, A., Le Fèvre, O., Mazure, A., Meneux, B., ...
The VIMOS VLT deep survey - the K-band follow-up in the 0226-04 field (2008)
Temporin, S., Iovino, A., Bolzonella, M., McCracken, H. J., Scodeggio, M., Garilli, B., ...
Optically selected type-2 AGN: preliminary results from the COSMOS survey (2008)
Bongiorno, A., Mignoli, M., Zamorani, G., Lamareille, F., Contini, T., ZCOSMOS Team
The VLA-COSMOS Survey. III. Further catalog analysis and the radio source counts (2008)
Bondi, M., Ciliegi, P., Schinnerer, E., Smolcic, V., Jahnke, K., Carilli, C., ...
The VLA-COSMOS Large Project has imaged the 2 deg2 COSMOS field with a resolution of 1.5" and a sensitivity of about 11 muJy (1 sigma), yielding a catalog of ~3600 radio sources. In this paper we...
Smolcic, V., Schinnerer, E., Scodeggio, M., Franzetti, P., Aussel, H., Bondi, M., ...
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 active galactic nucleus (AGN)...
A spectroscopic study of a z=1.6 galaxy overdensity in the GMASS field (2008)
Kurk, J., Cimatti, A., Zamorani, G., Halliday, C., Mignoli, M., Pozzetti, L., ...
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 peak at z = 1.6,...
GMASS, Unveiling Distant Massive Galaxies with Spitzer (2008)
Kurk, J. D., Cimatti, A., Daddi, E., Dickinson, M., Mignoli, M., Pozzetti, L., ...
One of the main questions of galaxy formation is how and when galaxies assembled their mass. Observations suggest that most mass assembly and star formation occured at 1 < z < 3. However, in the same...
GMASS ultradeep spectroscopy of galaxies at z ~ 2 . I. The stellar metallicity (2008)
Halliday, C., Daddi, E., Cimatti, A., Kurk, J., Renzini, A., Mignoli, M., ...
Context: Galaxy metallicities have been measured to redshift zÃÅ2 by gas-phase oxygen abundances of the interstellar medium using the R{23} and N2 methods. Galaxy stellar metallicities provide...
Cimatti, A., Cassata, P., Pozzetti, L., Kurk, J., Mignoli, M., Renzini, A., ...
Aims. The aim of this work is to investigate the physical, structural and evolutionary properties of old, passive galaxies at z > 1.4 and to place new constraints on massive galaxy formation and...
Cassata, P., Cimatti, A., Kurk, J., Rodighiero, G., Pozzetti, L., Bolzonella, M., ...
Aims. 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 1.42 we still find red galaxies in the...
Optically selected type-2 AGN: preliminary results from the COSMOS survey (2008)
Bongiorno, A., Mignoli, M., Zamorani, G., Lamareille, F., Contini, T., ZCOSMOS Team
Arnouts, S., Walcher, C. J., Le Fèvre, O., Zamorani, G., Ilbert, O., Le Brun, V., ...
We present an analysis of the stellar mass growth over the last 10 Gyr (z ≤ 2) using a unique large sample of galaxies selected at 3.6 μm. We have assembled accurate photometric and spectroscopic...
Clustering properties of a type-selected volume-limited sample of galaxies in the CFHTLS (2007)
McCracken, H. J., Ilbert, O., Mellier, Y., Bertin, E., Guzzo, L., Arnouts, S., ...
(abridged) We present an investigation of the clustering of i'AB
PSPC observations of the Shapley Supercluster: Abell 3562 (2007)
S. Ettori, S. Bardelli, S. De Grandi, S. Molendi, G. Zamorani, E. Zucca
We present a combined analysis of the BeppoSAX and ROSAT PSPC observation of the cluster of galaxies Abell 3562, a massive member of the core of the Shapley Supercluster. With a complex and...
The VIMOS-VLT Deep Survey. The dependence of clustering on galaxy stellar mass at z~1 (2007)
Meneux, B., Guzzo, L., Garilli, B., Fevre, O. Le, Pollo, A., Blaizot, J., ...
Aims: We use the VVDS-Deep first-epoch data to measure the dependence of galaxy clustering on galaxy stellar mass, at z~0.85. Methods: We measure the projected correlation function wp(rp) for...
Arnouts, S., Walcher, C. J., Le Fevre, O., Zamorani, G., Ilbert, O., Pozzetti, L., ...
(abridged abstract) We present an analysis of the stellar mass growth over the last 10 Gyrs using a large 3.6$\mu$ selected sample. We split our sample into active (blue) and quiescent (red)...
Vergani, D., Scodeggio, M., Pozzetti, L., Iovino, A., Franzetti, P., Garilli, B., ...
We select a mass limited sample of 4048 objects from the VIMOS VLT Deep Survey (VVDS) in the redshift interval 0.5
The VVDS type-1 AGN sample: The faint end of the luminosity function (2007)
Bongiorno, A., Zamorani, G., Gavignaud, I., Marano, B., Paltani, S., Mathez, G., ...
In a previous paper (Gavignaud et al. 2006), we presented the type-1 Active Galactic Nuclei (AGN) sample obtained from the first epoch data of the VIMOS-VLT Deep Survey (VVDS). The sample consists of...
Pozzetti, L., Bolzonella, M., Lamareille, F., Zamorani, G., Franzetti, P., Le Fevre, O., ...
We present a detailed analysis of the Galaxy Stellar Mass Function of galaxies up to z=2.5 as obtained from the VVDS. We estimate the stellar mass from broad-band photometry using 2 different...
Vergani, D., Scodeggio, M., Pozzetti, L., Iovino, A., Franzetti, P., Garilli, B., ...
We selected a mass-limited sample of 4048 objects from the VIMOS VLT Deep Survey in the redshift interval 0.5
Unveiling obscured accretion in the Chandra Deep Field South (2007)
Fiore, F., Grazian, A., Santini, P., Puccetti, S., Brusa, M., Feruglio, C., ...
A large population of heavily obscured, Compton Thick AGNs is predicted by models of galaxy formation, models of Cosmic X-ray Background and by the ``relic'' super-massive black-hole mass function...
Arnouts, S., Walcher, C. J., Fevre, O. Le, Zamorani, G., Ilbert, O., Brun, V. Le, ...
(abridged abstract) We present an analysis of the stellar mass growth over the last 10 Gyrs using a large 3.6$\mu$ selected sample. We split our sample into active (blue) and quiescent (red)...
The First Release COSMOS Optical and Near-IR Data and Catalog (2007)
Capak, P., Aussel, H., Ajiki, M., McCracken, H. J., Mobasher, B., Scoville, N., ...
We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3um and 2.4um. These include data taken on the Subaru 8.3m telescope, the KPNO and CTIO 4m telescopes,...
X-ray source counts in the COSMOS field (2007)
Cappelluti, N., Hasinger, G., Brusa, M., Comastri, A., Zamorani, G., Boehringer, H., ...
We present the analysis of the source counts in the XMM-COSMOS survey using data of the first year of XMM-Newton observations. The survey covers ~2 deg^2 within the region of sky bounded by 9^h57.5^m
Pozzetti, L., Bolzonella, M., Lamareille, F., Zamorani, G., Franzetti, P., Fèvre, O. Le, ...
We present a detailed analysis of the Galaxy Stellar Mass Function of galaxies up to z=2.5 as obtained from the VVDS. We estimate the stellar mass from broad-band photometry using 2 different...
The VVDS type-1 AGN sample: The faint end of the luminosity function (2007)
Bongiorno, A., Zamorani, G., Gavignaud, I., Marano, B., Paltani, S., Mathez, G., ...
In a previous paper (Gavignaud et al. 2006), we presented the type-1 Active Galactic Nuclei (AGN) sample obtained from the first epoch data of the VIMOS-VLT Deep Survey (VVDS). The sample consists of...
The obscured X-ray source population in the HELLAS2XMM survey: the Spitzer view (2007)
Vignali, C., Pozzi, Francesca, Comastri, A., Pozzetti, L., Mignoli, M., Gruppioni, C., ...
Recent X-ray surveys have provided a large number of high-luminosity, obscured Active Galactic Nuclei (AGN), the so-called Type 2 quasars. Despite the large amount of multi-wavelength supporting...
Pozzi, F., Vignali, C., Comastri, A., Pozzetti, L., Mignoli, M., Gruppioni, C., ...
Aims: We aim at estimating the spectral energy distributions (SEDs) and the physical parameters related to the black holes harbored in eight high X-ray-to-optical (F_X/F_R>10) obscured quasars at...
Spectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey (2007)
Polletta, M., Tajer, M., Maraschi, L., Trinchieri, G., Lonsdale, C. J., Chiappetti, L., ...
We present the spectral energy distributions (SEDs) of a hard X-ray selected sample. The sample contains 136 sources with F(2-10 keV)>10^-14 erg/cm^2/s and 132 are AGNs. The sources are detected in a...
Fevre, O. Le, Arnouts, S., Guzzo, L., Farrah, D., Iovino, A., ...
By combining the VVDS with the SWIRE data, we have built the currently largest spectroscopic sample of galaxies selected in the rest-frame near-infrared. These allow us to investigate, for the first...
The Zurich Extragalactic Bayesian Redshift Analyzer (ZEBRA) and its first application: COSMOS (2007)
Feldmann, R., Carollo, C. M., Porciani, C., Lilly, S. J., Capak, P., Taniguchi, Y., ...
We present ZEBRA, the Zurich Extragalactic Bayesian Redshift Analyzer. The current version of ZEBRA combines and extends several of the classical approaches to produce accurate photometric redshifts...
Finoguenov, A., Guzzo, L., Hasinger, G., Scoville, N. Z., Aussel, H., Boehringer, H., ...
We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the COSMOS field. We reach a depth for a total cluster flux in the 0.5-2 keV band of 3x10-15 ergs cm-2...
zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field (2007)
Lilly, S. J., Fevre, O. Le, Renzini, A., Zamorani, G., Scodeggio, M., Contini, T., ...
zCOSMOS is a large redshift survey that is being undertaken in the COSMOS field using 600 hours of observation with the VIMOS spectrograph on the 8-m VLT. The survey is designed to characterise the...
VVDS-SWIRE: Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2 (2007)
Fevre, O. Le, Arnouts, S., Guzzo, L., Farrah, D., Iovino, A., ...
By combining the VVDS with the SWIRE data, we have built the currently largest spectroscopic sample of galaxies selected in the rest-frame near-infrared. These allow us to investigate, for the first...
NIR Follow-Up of the VVDS 02hr Field (2007)
Temporin, S., Iovino, A., McCracken, H. J., Bolzonella, M., Scodeggio, M., Bottini, D., ...
We present a new K-band survey covering 623 arcmin$^2$ in the VVDS 0226-0430 deep field down to a limiting magnitude K$_{\rm{Vega}}$ $\leq$ 20.5. We use the spectroscopic sample extracted from this...
Witnessing the build-up of the colour-density relation (2007)
Cucciati, O., Iovino, A., Marinoni, C., Ilbert, O., Bardelli, S., Franzetti, P., ...
We investigate the redshift and luminosity evolution of the galaxy colour-density relation using the data from the First Epoch VIMOS-VLT Deep Survey (VVDS) on scales of R=5 h^(-1)Mpc up to redshift z...
The VIRMOS-VLT Deep Survey: the last 10 billion years of evolution of galaxy clustering (2007)
Pollo, A., Guzzo, L., Fevre, O. Le, Meneux, B., Cappi, A., McCracken, H. J., ...
We discuss the evolution of clustering of galaxies in the Universe from the present epoch back to z ~ 2, using the first-epoch data from the VIMOS-VLT Deep Survey (VVDS). We present the evolution of...
Studying the Evolution of Multi-Wavelength Emissivities with the Vimos VLT Deep Survey (2007)
Tresse, L., Ilbert, O., Zucca, E., Zamorani, G., Arnouts, S., Bardelli, S., ...
The VIMOS VLT Deep Survey is a unique I-selected spectroscopic sample to study galaxies all the way from z=5 to z=0. We recapitulate the first results about the evolution of the galaxy populations as...
The VIMOS-VLT Deep Survey. Beyond color bimodality: the mix of galaxy populations up to z~2 (2007)
Franzetti, P., Scodeggio, M., Maccagni, D., Garilli, B., Vergani, D., Guzzo, L., ...
In this paper we discuss the mix of star-forming and passive galaxies up to z~2, based on the first epoch VIMOS-VLT Deep Survey (VVDS) data.In agreement with previous works we find that the galaxy...
Paltani, S., Fevre, O. Le, Ilbert, O., Arnouts, S., Bardelli, S., Tresse, L., ...
We study the LF of the high-z galaxy population with 3
The cosmic star formation rate evolution from z=5 to z=0 from the VIMOS VLT Deep Survey (2007)
Tresse, L., Ilbert, O., Zucca, E., Zamorani, G., Bardelli, S., Arnouts, S., ...
We present the evolution of the SFRD in the redshift range 0
The XMM-Newton wide-field survey in the COSMOS field II: X-ray data and the logN-logS (2007)
Cappelluti, N., Hasinger, G., Brusa, M., Comastri, A., Zamorani, G., Boehringer, H., ...
We present the data analysis and the X-ray source counts for the first season of XMM-Newton observations in the COSMOS field. The survey covers ~2 deg^2 within the region of sky bounded by 9^h57.5^m
The XMM-Newton survey in the Marano field - I. The X-ray data and optical follow-up (2007)
Krumpe, M., Lamer, G., Schwope, A. D., Wagner, S., Zamorani, G., Mignoli, M., ...
The VVDS type-1 AGN sample: the faint end of the luminosity function (2007)
Bongiorno, A., Zamorani, G., Gavignaud, I., Marano, B., Paltani, S., Mathez, G., ...
The first release COSMOS optical and near-IR data and catalog (2007)
Capak, P., Aussel, H., Ajiki, M., McCracken, H. J., Mobasher, B., Scoville, N., ...
zCOSMOS: a large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field (2007)
Lilly, S. J., Le Fèvre, O., Renzini, A., Zamorani, G., Scodeggio, M., Contini, T., ...
The XMM-Newton wide-field survey in the COSMOS field - I. Survey description (2007)
Hasinger, G., Cappelluti, N., Brunner, H., Brusa, M., Comastri, A., Elvis, M., ...
Le Fèvre, O., Arnouts, S., Guzzo, L., Farrah, D., Iovino, A., ...
The VIMOS VLT deep survey: clustering and the role of environment in galaxy evolution (2007)
Le Fèvre, O., Cucciati, O., Guzzo, L., Ilbert, O., Iovino, A., Marinoni, C., ...
X-ray source counts in the XMM-COSMOS survey (2007)
Cappelluti, N., Hasinger, G., Brusa, M., Comastri, A., Zamorani, G., Böhringer, H., ...
X-ray source counts in the XMM-COSMOS survey (2007)
Cappelluti, N., Hasinger, G., Brusa, M., Comastri, A., Zamorani, G., Böhringer, H., ...
The VIMOS-VLT deep survey: the last 10 billion years of evolution of galaxy clustering (2007)
Pollo, A., Guzzo, L., Le Fèvre, O., Meneux, B., Cappi, A., McCracken, H. J., ...
Mainieri, V., Hasinger, G., Cappelluti, N., Brusa, M., Brunner, H., Civano, F., ...
We present a detailed spectral analysis of pointlike X-ray sources in the XMM-Newton COSMOS field. Our sample of 135 sources only includes those that have more than 100 net counts in the 0.3-10 keV...
zCOSMOS: a large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field (2007)
Lilly, S. J., Le Fevre, O., Renzini, A., Zamorani, G., Scodeggio, M., Contini, T., ...
zCOSMOS is a large redshift survey that is being undertaken in the COSMOS field using 600 hours of observation with the VIMOS spectrograph on the 8-m VLT. The survey is designed to characterise the...
Finoguenov, A., Guzzo, L., Hasinger, G., Scoville, N. Z., Aussel, H., Böhringer, H., ...
We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the Cosmic Evolution Survey (COSMOS) field. We reach a depth for a total cluster flux in the 0.5-2 keV...
The first release COSMOS optical and Near-IR data and catalog (2007)
Capak, P., Aussel, H., Ajiki, M., McCracken, H. J., Mobasher, B., Scoville, N., ...
We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3 and 2.4 mum. These include data taken on the Subaru 8.3 m telescope, the KPNO and CTIO 4 m telescopes,...
Pollo, A., Abbas, U., Meneux, B., Guzzo, L., Le Fèvre, O., Cappi, A., ...
Pollo, A., Abbas, U., Meneux, B., Guzzo, L., Le Fèvre, O., Cappi, A., ...
Highlights from the VIMOS VLT Deep Survey (2007)
Le Fevre, O., Garilli, B., Le Brun, V., Maccagni, D., Scaramella, R., Scodeggio, M., ...
Redshift-space distortions as a probe of dark energy (2007)
Guzzo, L., Pierleoni, M., Meneux, B., Branchini, E., Le Fèvre, O., Marinoni, C., ...
Polletta, M, Tajer, M, Maraschi, L, Trinchieri, G, Lonsdale, C J, Chiappetti, L, ...
We present the SEDs of a hard X-ray selected sample containing 136 sources with F[SUB]2-10keV[/SUB]>10[SUP]-14[/SUP] erg cm[SUP]-2[/SUP] s[SUP]-1[/SUP] 132 are AGNs. The sources are detected in a 1...
Brusa, M., Zamorani, G., Comastri, A., Hasinger, G., Cappelluti, N., Civano, F., ...
[ABRIGED] We present the optical identification of a sample of 695 X-ray sources detected in the first 1.3 deg^2 of the XMM-COSMOS survey, down to a 0.5-2 keV (2-10 keV) limiting flux of ~10^-15 erg...
Finoguenov, A., Guzzo, L., Hasinger, G., Scoville, N. Z., Aussel, H., Boehringer, H., ...
We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the COSMOS field. We reach a depth for a total cluster flux in the 0.5-2 keV band of 3x10-15 ergs cm-2...
Mainieri, V., Hasinger, G., Cappelluti, N., Brusa, M., Brunner, H., Civano, F., ...
We present a detailed spectral analysis of point-like X-ray sources in the XMM-COSMOS field. Our sample of 135 sources only includes those that have more than 100 net counts in the 0.3-10 keV energy...
The VIRMOS-VLT Deep Survey: the last 10 billion years of evolution of galaxy clustering (2006)
Pollo, A., Guzzo, L., Fevre, O. Le, Meneux, B., Cappi, A., McCracken, H. J., ...
We discuss the evolution of clustering of galaxies in the Universe from the present epoch back to z ~ 2, using the first-epoch data from the VIMOS-VLT Deep Survey (VVDS). We present the evolution of...
The XMM-Newton Survey in the Marano Field I. The X-ray data and optical follow-up (2006)
Krumpe, M., Lamer, G., Schwope, A. D., Wagner, S., Zamorani, G., Mignoli, M., ...
We report on a medium deep XMM-Newton survey of the Marano Field and optical follow-up observations. The mosaicked XMM-Newton pointings in this optical quasar survey field cover 0.6 square degree...
COSMOS : Hubble Space Telescope Observations (2006)
Scoville, N., Benson, A., Blain, A. W., Calzetti, D., Comastri, A., Capak, P., ...
The Cosmic Evolution Survey (COSMOS) was initiated with an extensive allocation (590 orbits in Cycles 12-13) using the Hubble Space Telescope (HST) for high resolution imaging. Here we review the...
The XMM-Newton wide-field survey in the COSMOS field: I. Survey description (2006)
Hasinger, G., Cappelluti, N., Brunner, H., Brusa, M., Comastri, A., Elvis, M., ...
We present the first set of XMM-Newton EPIC observations in the 2 square degree COSMOS field. The strength of the COSMOS project is the unprecedented combination of a large solid angle and...
zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field (2006)
Lilly, S. J., Fevre, O. Le, Renzini, A., Zamorani, G., Scodeggio, M., Contini, T., ...
zCOSMOS is a large redshift survey that is being undertaken in the COSMOS field using 600 hours of observation with the VIMOS spectrograph on the 8-m VLT. The survey is designed to characterise the...
Witnessing the build-up of the colour-density relation (2006)
Cucciati, O., Iovino, A., Marinoni, C., Ilbert, O., Bardelli, S., Franzetti, P., ...
We investigate the redshift and luminosity evolution of the galaxy colour-density relation using the data from the First Epoch VIMOS-VLT Deep Survey (VVDS) on scales of R=5 h^(-1)Mpc up to redshift z...
Studying the Evolution of Multi-Wavelength Emissivities with the Vimos VLT Deep Survey (2006)
Tresse, L., Ilbert, O., Zucca, E., Zamorani, G., Arnouts, S., Bardelli, S., ...
The VIMOS VLT Deep Survey is a unique I-selected spectroscopic sample to study galaxies all the way from z=5 to z=0. We recapitulate the first results about the evolution of the galaxy populations as...
NIR Follow-Up of the VVDS 02hr Field (2006)
Temporin, S., Iovino, A., McCracken, H. J., Bolzonella, M., Scodeggio, M., Bottini, D., ...
We present a new K-band survey covering 623 arcmin$^2$ in the VVDS 0226-0430 deep field down to a limiting magnitude K$_{\rm{Vega}}$ $\leq$ 20.5. We use the spectroscopic sample extracted from this...
The Zurich Extragalactic Bayesian Redshift Analyzer and its first application: COSMOS (2006)
Feldmann, R., Carollo, C. M., Porciani, C., Lilly, S. J., Capak, P., Taniguchi, Y., ...
We present the Zurich Extragalactic Bayesian Redshift Analyzer (ZEBRA). The current version of ZEBRA combines and extends several of the classical approaches to produce accurate photometric redshifts...
The Zurich Extragalactic Bayesian Redshift Analyzer (ZEBRA) and its first application: COSMOS (2006)
Feldmann, R., Carollo, C. M., Porciani, C., Lilly, S. J., Capak, P., Taniguchi, Y., ...
We present ZEBRA, the Zurich Extragalactic Bayesian Redshift Analyzer. The current version of ZEBRA combines and extends several of the classical approaches to produce accurate photometric redshifts...
The cosmic star formation rate evolution from z=5 to z=0 from the VIMOS VLT Deep Survey (2006)
Tresse, L., Ilbert, O., Zucca, E., Zamorani, G., Bardelli, S., Arnouts, S., ...
We present the evolution of the comoving SFR density in the redshift range 0 < z < 5 using the first epoch data release of the VVDS, that is 11564 spectra selected at I_AB=24 over 2200 arcmin^2 in...
Paltani, S., Fevre, O. Le, Ilbert, O., Arnouts, S., Bardelli, S., Tresse, L., ...
We study the LF of the high-z galaxy population with 3
Puccetti, S., Fiore, F., D'Elia, V., Pillitteri, I., Feruglio, C., Grazian, A., ...
We have surveyed with XMM-Newton the central ~0.6 deg2 region of the ELAIS-S1 field down to flux limits of ~5.5X10-16 cgs (0.5-2 keV, S band), ~2X10-15 cgs (2-10 keV, H band), and ~4X10-15 cgs (5-10...
The VIMOS-VLT Deep Survey. Color bimodality and the mix of galaxy populations up to z~2 (2006)
Franzetti, P., Scodeggio, M., Garilli, B., Vergani, D., Maccagni, D., Guzzo, L., ...
In this paper we discuss the mix of star-forming and passive galaxies up to z~2, based on the first epoch VIMOS-VLT Deep Survey (VVDS) data.In agreement with previous works we find that the galaxy...
Zucca, E., Ilbert, O., Bardelli, S., Tresse, L., Zamorani, G., Arnouts, S., ...
From the first epoch observations of the VVDS up to z=1.5 we have derived luminosity functions (LF) of different spectral type galaxies. The VVDS data, covering ~70% of the life of the Universe,...
The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5 (2006)
Meneux, B., LeFevre, O., Guzzo, L., Pollo, A., Cappi, A., Ilbert, O., ...
We measure the evolution of clustering for galaxies with different spectral types from 6495 galaxies with 17.5
Ilbert, O., Cucciati, O., Marinoni, C., Tresse, L., Fevre, O. Le, Zamorani, G., ...
We measure the evolution of the galaxy Luminosity Function as a function of large-scale environment up to z=1.5 from the VIMOS-VLT Deep Survey (VVDS) first epoch data. The 3D galaxy density field is...
The VIMOS VLT Deep Survey: The build-up of the colour-density relation (2006)
Cucciati, O., Iovino, A., Marinoni, C., Ilbert, O., Bardelli, S., Franzetti, P., ...
We investigate the redshift and luminosity evolution of the galaxy colour-density relation using the data from the First Epoch VIMOS-VLT Deep Survey (VVDS). The size (6582 galaxies), depth (I_AB
Ilbert, O., Arnouts, S., McCracken, H. J., Bolzonella, M., Bertin, E., Fevre, O. Le, ...
We present photometric redshifts for an uniquely large and deep sample of 522286 objects with i'_{AB}
Galaxy luminosity function per morphological type up to z=1.2 (2006)
Ilbert, O., Lauger, S., Tresse, L., Buat, V., Arnout, S., Fevre, O. Le, ...
We have computed the evolution of the rest-frame B-band luminosity function (LF) for bulge and disk-dominated galaxies since z=1.2. We use a sample of 605 spectroscopic redshifts with I_{AB}0.9 and...
The VIMOS VLT Deep Survey: the faint type-1 AGN sample (2006)
Gavignaud, I., Bongiorno, A., Paltani, S., Mathez, G., Zamorani, G., Moller, P., ...
We present the type-1 active galactic nuclei (AGN) sample extracted from the VIMOS VLT Deep Survey first observations of 21000 spectra in 1.75 square degree. This sample, which is purely magnitude...
The VIMOS VLT Deep Survey: Public release of 1599 redshifts to IAB (2006)
Fevre, O. Le, Vettolani, G., Paltani, S., Tresse, L., Zamorani, G., Brun, V. Le, ...
{This paper presents the VIMOS VLT Deep Survey around the Chandra Deep Field South (CDFS). We have measured 1599 new redshifts with VIMOS on the European Observatory Very Large Telescope - UT3, in an...
The VIRMOS deep imaging survey: III. ESO/WFI deep U-band imaging of the 0226-04 deep field (2006)
Radovich, M., Arnaboldi, M., Ripepi, V., Massarotti, M., McCracken, H. J., Mellier, Y., ...
In this paper we describe the U-band imaging of the F02 deep field, one of the fields in the VIRMOS Deep Imaging Survey. The observations were done at the ESO/MPG 2.2m telescope at La Silla (Chile)...
The VIMOS VLT Deep Survey: the faint type-1 AGN sample (2006)
Gavignaud, I., Bongiorno, A., Paltani, S., Mathez, G., Zamorani, G., Moller, P., ...
We present the type-1 active galactic nuclei (AGN) sample extracted from the VIMOS VLT Deep Survey first observations of 21000 spectra in 1.75 square degree. This sample, which is purely magnitude...
GMASS, Unveiling Distant Massive Galaxies with Spitzer (2006)
Kurk, J. D., Cimatti, A., Daddi, E., Dickinson, M., Mignoli, M., Pozzetti, L., ...
One of the main questions of galaxy formation is how and when galaxies assembled their mass. Observations suggest that most mass assembly and star formation occured at 1 < z < 3. However, in the same...
Galaxy luminosity function per morphological type up to z=1.2 (2006)
Ilbert, O., Lauger, S., Tresse, L., Buat, V., Arnout, S., Fevre, O. Le, ...
We have computed the evolution of the rest-frame B-band luminosity function (LF) for bulge and disk-dominated galaxies since z=1.2. We use a sample of 605 spectroscopic redshifts with I_{AB}0.9 and...
The VIMOS VLT Deep Survey: The build-up of the colour-density relation (2006)
Cucciati, O., Iovino, A., Marinoni, C., Ilbert, O., Bardelli, S., Franzetti, P., ...
We investigate the redshift and luminosity evolution of the galaxy colour-density relation using the data from the First Epoch VIMOS-VLT Deep Survey (VVDS). The size (6582 galaxies), depth (I_AB
Ilbert, O., Arnouts, S., McCracken, H. J., Bolzonella, M., Bertin, E., Fevre, O. Le, ...
We present photometric redshifts for an uniquely large and deep sample of 522286 objects with i'_{AB}
Ilbert, O., Cucciati, O., Marinoni, C., Tresse, L., Fevre, O. Le, Zamorani, G., ...
We measure the evolution of the galaxy Luminosity Function as a function of large-scale environment up to z=1.5 from the VIMOS-VLT Deep Survey (VVDS) first epoch data. The 3D galaxy density field is...
Pollo, A., Meneux, B., Guzzo, L., Fevre, O. Le, Blaizot, J., Cappi, A., ...
We are presenting in this paper a detailed account of the methods used to compute the three-dimensional two-point galaxy correlation function in the VIMOS-VLT deep survey (VVDS). We investigate how...
The Very Large Telescope Visible Multi-Object Spectrograph Mask Preparation Software (2006)
Bottini, D., Garilli, B., Maccagni, D., Tresse, L., Le Brun, V., Le Fèvre, O., ...
VIMOS (Visible Multi-Object Spectrograph) is a multiobject imaging spectrograph installed at the VLT (Very large Telescope) at the ESO (European Southern Observatory) Paranal Observatory that is...
A large population of galaxies 9 to 12 billion years back in the history of the Universe (2006)
Le Fevre, O., Paltani, S., Arnouts, S., Charlot, S., Foucaud, S., Ilbert, O., ...
To understand the evolution of galaxies, we need to know as accurately as possible how many galaxies were present in the Universe at different epochs. Galaxies in the young Universe have hitherto...
The VIMOS VLT Deep Survey - First epoch VVDS-Deep survey: 11564 spectra with 17.5 (2006)
Le Fevre, O., Vettolani, G., Garilli, B., Tresse, L., Maccagni, D., ...
This paper presents the ``First Epoch\'\' sample from the VIMOS VLT Deep Survey (VVDS). The VVDS goals, observations, data reduction with VIPGI, and redshift measurement with KBRED are discussed....
Le Fevre, O., Guzzo, L., Meneux, B., Pollo, A., Cappi, A., Colombi, S., ...
This paper presents the evolution of the clustering of the main population of galaxies from z=2.1 to z=0.2, from the first epoch VIMOS VLT Deep Survey (VVDS), a magnitude limited sample with 17.5
Matute, I., La Franca, F., Pozzi, F., Gruppioni, C., Lari, C., Zamorani, G.
We study the evolution of the luminosity function (LF) of type-1 and type-2 AGN in the mid-infrared, and derive their contribution to the Cosmic InfraRed Background (CIRB) and the expected deep...
Zucca, E., Ilbert, O., Bardelli, S., Tresse, L., Zamorani, G., Arnouts, S., ...
From the first epoch observations of the VVDS up to z=1.5 we have derived luminosity functions (LF) of different spectral type galaxies. The VVDS data, covering ~70% of the life of the Universe,...
The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5 (2006)
Meneux, B., LeFevre, O., Guzzo, L., Pollo, A., Cappi, A., Ilbert, O., ...
We measure the evolution of clustering for galaxies with different spectral types from 6495 galaxies with 17.5
Ilbert, O., Cucciati, O., Marinoni, C., Tresse, L., Fevre, O. Le, Zamorani, G., ...
We measure the evolution of the galaxy Luminosity Function as a function of large-scale environment up to z=1.5 from the VIMOS-VLT Deep Survey (VVDS) first epoch data. The 3D galaxy density field is...
The VIMOS VLT Deep Survey: The build-up of the colour-density relation (2006)
Cucciati, O., Iovino, A., Marinoni, C., Ilbert, O., Bardelli, S., Franzetti, P., ...
We investigate the redshift and luminosity evolution of the galaxy colour-density relation using the data from the First Epoch VIMOS-VLT Deep Survey (VVDS). The size (6582 galaxies), depth (I_AB
Ilbert, O., Arnouts, S., McCracken, H. J., Bolzonella, M., Bertin, E., Fevre, O. Le, ...
We present photometric redshifts for an uniquely large and deep sample of 522286 objects with i'_{AB}
Galaxy luminosity function per morphological type up to z=1.2 (2006)
Ilbert, O., Lauger, S., Tresse, L., Buat, V., Arnout, S., Fevre, O. Le, ...
We have computed the evolution of the rest-frame B-band luminosity function (LF) for bulge and disk-dominated galaxies since z=1.2. We use a sample of 605 spectroscopic redshifts with I_{AB}0.9 and...
The VIMOS VLT Deep Survey: the faint type-1 AGN sample (2006)
Gavignaud, I., Bongiorno, A., Paltani, S., Mathez, G., Zamorani, G., Moller, P., ...
We present the type-1 active galactic nuclei (AGN) sample extracted from the VIMOS VLT Deep Survey first observations of 21000 spectra in 1.75 square degree. This sample, which is purely magnitude...
Zucca, E., Ilbert, O., Bardelli, S., Tresse, L., Zamorani, G., Arnouts, S., ...
From the first epoch observations of the VVDS up to z=1.5 we have derived luminosity functions (LF) of different spectral type galaxies. The VVDS data, covering ~70% of the life of the Universe,...
The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5 (2006)
Meneux, B., LeFevre, O., Guzzo, L., Pollo, A., Cappi, A., Ilbert, O., ...
We measure the evolution of clustering for galaxies with different spectral types from 6495 galaxies with 17.5
Ilbert, O., Cucciati, O., Marinoni, C., Tresse, L., Fevre, O. Le, Zamorani, G., ...
We measure the evolution of the galaxy Luminosity Function as a function of large-scale environment up to z=1.5 from the VIMOS-VLT Deep Survey (VVDS) first epoch data. The 3D galaxy density field is...
The VIMOS VLT Deep Survey: The build-up of the colour-density relation (2006)
Cucciati, O., Iovino, A., Marinoni, C., Ilbert, O., Bardelli, S., Franzetti, P., ...
We investigate the redshift and luminosity evolution of the galaxy colour-density relation using the data from the First Epoch VIMOS-VLT Deep Survey (VVDS). The size (6582 galaxies), depth (I_AB
Ilbert, O., Arnouts, S., McCracken, H. J., Bolzonella, M., Bertin, E., Fevre, O. Le, ...
We present photometric redshifts for an uniquely large and deep sample of 522286 objects with i'_{AB}
Galaxy luminosity function per morphological type up to z=1.2 (2006)
Ilbert, O., Lauger, S., Tresse, L., Buat, V., Arnout, S., Fevre, O. Le, ...
We have computed the evolution of the rest-frame B-band luminosity function (LF) for bulge and disk-dominated galaxies since z=1.2. We use a sample of 605 spectroscopic redshifts with I_{AB}0.9 and...
The VIMOS VLT Deep Survey: the faint type-1 AGN sample (2006)
Gavignaud, I., Bongiorno, A., Paltani, S., Mathez, G., Zamorani, G., Moller, P., ...
We present the type-1 active galactic nuclei (AGN) sample extracted from the VIMOS VLT Deep Survey first observations of 21000 spectra in 1.75 square degree. This sample, which is purely magnitude...
X-ray emitting eros as tracers of black holes-galaxies coevolution (2006)
Brusa, M., Comastri, A., Daddi, E., Mignoli, M., Vignali, C., Zamorani, G., ...
Meneux, B., Le Fèvre, O., Guzzo, L., Pollo, A., Cappi, A., Ilbert, O., ...
The VIMOS-VLT deep survey - galaxy luminosity function per morphological type up to z = 1.2 (2006)
Ilbert, O., Lauger, S., Tresse, L., Buat, V., Arnouts, S., Le Fèvre, O., ...
The VIMOS VLT deep survey: the faint type-1 AGN sample (2006)
Gavignaud, I., Bongiorno, A., Paltani, S., Mathez, G., Zamorani, G., Møller, P., ...
The Zurich Extragalactic Bayesian Redshift Analyzer and its first application: COSMOS (2006)
Feldmann, R., Carollo, C. M., Porciani, C., Lilly, S. J., Capak, P., Taniguchi, Y., ...
Scodeggio, M., Franzetti, P., Garilli, B., Zanichelli, A., Paltani, S., Maccagni, D., ...
The VIMOS VLT Deep Survey (VVDS), designed to measure 150,000 galaxy redshifts, requires a dedicated data reduction and analysis pipeline to process in a timely fashion the large amount of...
Schiminovich, D., Ilbert, O., Arnouts, S., Milliard, B., Tresse, L., Fevre, O. Le, ...
In a companion paper (Arnouts et al. 2004) we presented new measurements of the galaxy luminosity function at 1500 Angstroms out to z~1 using GALEX-VVDS observations (1039 galaxies with NUV0.2) and...
Ilbert, O., Tresse, L., Zucca, E., Bardelli, S., Arnouts, S., Zamorani, G., ...
We investigate the evolution of the galaxy luminosity function from the VIMOS-VLT Deep Survey (VVDS) from the present to z=2 in five (U, B, V, R and I) rest-frame band-passes. We use the first epoch...
The VIMOS Integral Field Unit: data reduction methods and quality assessment (2005)
Zanichelli, A., Garilli, B., Scodeggio, M., Franzetti, P., Rizzo, D., Maccagni, D., ...
With new generation spectrographs integral field spectroscopy is becoming a widely used observational technique. The Integral Field Unit of the VIsible Multi-Object Spectrograph on the ESO-VLT allows...
The VIRMOS deep imaging survey IV: Near-infrared observations (2005)
Iovino, A., McCracken, H. J., Garilli, B., Foucaud, S., Fevre, O. Le, Maccagni, D., ...
In this paper we present a new deep, wide-field near-infrared imaging survey. Our J- and K-band observations in four separate fields complement optical BVRI, ultraviolet and spectroscopic...
The VIMOS VLT Deep Survey: Evolution of the non-linear galaxy bias up to z=1.5 (2005)
Marinoni, C., Fevre, O. Le, Meneux, B., Iovino, A., Pollo, A., Ilbert, O., ...
We present the first measurements of the Probability Distribution Function (PDF) of galaxy fluctuations in the VIMOS-VLT Deep Survey (VVDS) cone, covering 0.4x0.4 deg between 0.4
Ciliegi, P., Zamorani, G., Bondi, M., Pozzetti, L., Bolzonella, M., Gregorini, L., ...
In this paper we present the optical and near-infrared identifications of the 1054 radio sources detected in the 20cm deep radio survey down to a 5sigma flux limit of about 80 microJy obtained with...
The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5 (2005)
Meneux, B., LeFevre, O., Guzzo, L., Pollo, A., Cappi, A., Ilbert, O., ...
We measure the evolution of clustering for galaxies with different spectral types from 6495 galaxies with 17.5
A large population of galaxies 9 to 12 billion years back in the history of the Universe (2005)
Fevre, O. Le, Paltani, S., Arnouts, S., Charlot, S., Foucaud, S., Ilbert, O., ...
To understand the evolution of galaxies, we need to know as accurately as possible how many galaxies were present in the Universe at different epochs. Galaxies in the young Universe have hitherto...
The VIMOS Integral Field Unit: data reduction methods and quality assessment (2005)
Zanichelli, A., Garilli, B., Scodeggio, M., Franzetti, P., Rizzo, D., Maccagni, D., ...
With new generation spectrographs integral field spectroscopy is becoming a widely used observational technique. The Integral Field Unit of the VIsible Multi-Object Spectrograph on the ESO-VLT allows...
Bias in the Estimation of Global Luminosity Functions (2005)
Ilbert, O., Tresse, L., Arnouts, S., Zucca, E., Bardelli, S., Zamorani, G., ...
We discuss a bias present in the calculation of the global luminosity function (LF) which occurs when analysing faint galaxy samples. This effect exists because of the different spectral energy...
The VLA-VIRMOS Deep Field I. Radio observations probing the microJy source population (2005)
Ciliegi, M. Bondi. P., Zamorani, G., Gregorini, L., Vettolani, G., Parma, P., De Ruiter, H., ...
We have conducted a deep survey (r.m.s noise 17 microJy) with the Very Large Array (VLA) at 1.4 GHz, with a resolution of 6 arcsec, of a 1 square degree region included in the VIRMOS VLT Deep Survey....
The VIRMOS deep imaging survey IV: Near-infrared observations (2005)
Iovino, A., McCracken, H. J., Garilli, B., Foucaud, S., Fevre, O. Le, Maccagni, D., ...
In this paper we present a new deep, wide-field near-infrared imaging survey. Our J- and K-band observations in four separate fields complement optical BVRI, ultraviolet and spectroscopic...
Ciliegi, P., Zamorani, G., Bondi, M., Pozzetti, L., Bolzonella, M., Garilli, L. Gregorini B., ...
In this paper we present the optical and near-infrared identifications of the 1054 radio sources detected in the 20cm deep radio survey down to a 5sigma flux limit of about 80 microJy obtained with...
The evolution of early-type galaxies at z~1 from the K20 survey (2005)
Alighieri, S. Di Serego, Vernet, J., Cimatti, A., Lanzoni, B., Cassata, P., Ciotti, L., ...
We have performed VLT spectroscopy of an almost complete sample of 18 early-type galaxies with 0.88 < z < 1.3 plus two at z=0.67, selected from the K20 survey, and derived the velocity dispersion for...
The VIMOS VLT Deep Survey: Evolution of the non-linear galaxy bias up to z=1.5 (2005)
Marinoni, C., Fevre, O. Le, Meneux, B., Iovino, A., Pollo, A., Ilbert, O., ...
We present the first measurements of the Probability Distribution Function (PDF) of galaxy fluctuations in the VIMOS-VLT Deep Survey (VVDS) cone, covering 0.4x0.4 deg between 0.4
Zucca, E., Ilbert, O., Bardelli, S., Tresse, L., Zamorani, G., Arnouts, S., ...
From the first epoch observations of the VVDS up to z=1.5 we have derived luminosity functions (LF) of different spectral type galaxies. The VVDS data, covering ~70% of the life of the Universe,...
Mignoli, M., Cimatti, A., Zamorani, G., Pozzetti, L., Daddi, E., Renzini, A., ...
The K20 survey is a near infrared-selected, deep (Ks < 20) redshift survey targeting galaxies in two independent regions of the sky, the CDFS and the q0055-2659 field. The total Ks-selected sample...
The Vimos-VLT Deep Survey: Results from the First-Epoch Observations (2005)
Le Fèvre, O., Marinoni, C., Garilli, B., Le Brun, V., Maccagni, D., ...
The Vimos-VLT Deep Survey is a spectroscopic survey aiming at collecting more than 50000 spectra down to a limiting magnitude IAB=24, and 100000 down to IAB=22.5, on a total of about 16 deg2 without...
Ciliegi, P., Zamorani, G., Bondi, M., Pozzetti, L., Bolzonella, M., Gregorini, L., ...
In this paper we present the optical and near-infrared identifications of the 1054 radio sources detected in the 20 cm deep radio survey down to a 5sigma flux limit of ~80 muJy obtained with the VLA...
Star-forming Galaxies in the VVDS-VLA-02h Deep Field (2005)
Bolzonella, M., Bondi, M., Bongiorno, A., Bottini, D., Busarello, G., Ciliegi, P., ...
Pollo, A., Meneux, B., Guzzo, L., Fevre, O. Le, Blaizot, J., Cappi, A., ...
We are presenting in this paper a detailed account of the methods used to compute the three-dimensional two-point galaxy correlation function in the VIMOS-VLT deep survey (VVDS). We investigate how...
The VIMOS VLT Deep Survey: A new window on the distant universe (2005)
Le Fèvre, O., Vettolani, G., Garilli, B., Tresse, L., Bottini, D., Le Brun, V., ...
The First Epoch VIMOS VLT Deep Survey is now completed. More than 11000 redshifts of galaxies with 17.5 ≤ IAB ≤ 24 have been measured with the VIMOS spectrograph build for ESO by our...
A large population of galaxies 9 to 12 billion years back in the history of the Universe (2005)
Le Fevre, O., Paltani, S., Arnouts, S., Charlot, S., Foucaud, S., Ilbert, O., ...
To understand the evolution of galaxies, we need to know as accurately as possible how many galaxies were present in the Universe at different epochs. Galaxies in the young Universe have hitherto...
The VIMOS VLT Deep Survey - First epoch VVDS-Deep survey: 11564 spectra with 17.5 (2005)
Le Fevre, O., Vettolani, G., Garilli, B., Tresse, L., Maccagni, D., ...
This paper presents the ``First Epoch\'\' sample from the VIMOS VLT Deep Survey (VVDS). The VVDS goals, observations, data reduction with VIPGI, and redshift measurement with KBRED are discussed....
Le Fevre, O., Guzzo, L., Meneux, B., Pollo, A., Cappi, A., Colombi, S., ...
This paper presents the evolution of the clustering of the main population of galaxies from z=2.1 to z=0.2, from the first epoch VIMOS VLT Deep Survey (VVDS), a magnitude limited sample with 17.5
The Very Large Telescope Visible Multi-Object Spectrograph Mask Preparation Software (2005)
Adami, C., Arnaboldi, M., Arnouts, S., Bardelli, S., Bolzonella, M., Bottini, D., ...
VIMOS (Visible Multi-Object Spectrograph) is a multiobject imaging spectrograph installed at the VLT (Very large Telescope) at the ESO (European Southern Observatory) Paranal Observatory that is...
Ilbert, O., Tresse, L., Zucca, E., Bardelli, S., Arnouts, S., Zamorani, G., ...
We investigate the evolution of the galaxy luminosity function from the VIMOS-VLT Deep Survey (VVDS) from the present to z=2 in five (U, B, V, R and I) rest-frame band-passes. We use the first epoch...
The VIMOS Integral Field Unit: data reduction methods and quality assessment (2005)
Zanichelli, A., Garilli, B., Scodeggio, M., Franzetti, P., Rizzo, D., Maccagni, D., ...
With new generation spectrographs integral field spectroscopy is becoming a widely used observational technique. The Integral Field Unit of the VIsible Multi-Object Spectrograph on the ESO-VLT allows...
The VIRMOS deep imaging survey IV: Near-infrared observations (2005)
Iovino, A., McCracken, H. J., Garilli, B., Foucaud, S., Fevre, O. Le, Maccagni, D., ...
In this paper we present a new deep, wide-field near-infrared imaging survey. Our J- and K-band observations in four separate fields complement optical BVRI, ultraviolet and spectroscopic...
The VIMOS VLT Deep Survey: Evolution of the non-linear galaxy bias up to z=1.5 (2005)
Marinoni, C., Fevre, O. Le, Meneux, B., Iovino, A., Pollo, A., Ilbert, O., ...
We present the first measurements of the Probability Distribution Function (PDF) of galaxy fluctuations in the VIMOS-VLT Deep Survey (VVDS) cone, covering 0.4x0.4 deg between 0.4
Ciliegi, P., Zamorani, G., Bondi, M., Pozzetti, L., Bolzonella, M., Gregorini, L., ...
In this paper we present the optical and near-infrared identifications of the 1054 radio sources detected in the 20cm deep radio survey down to a 5sigma flux limit of about 80 microJy obtained with...
Pollo, A., Meneux, B., Guzzo, L., Fevre, O. Le, Blaizot, J., Cappi, A., ...
We are presenting in this paper a detailed account of the methods used to compute the three-dimensional two-point galaxy correlation function in the VIMOS-VLT deep survey (VVDS). We investigate how...
A large population of galaxies 9 to 12 billion years back in the history of the Universe (2005)
Le Fevre, O., Paltani, S., Arnouts, S., Charlot, S., Foucaud, S., Ilbert, O., ...
To understand the evolution of galaxies, we need to know as accurately as possible how many galaxies were present in the Universe at different epochs. Galaxies in the young Universe have hitherto...
The VIMOS VLT Deep Survey - First epoch VVDS-Deep survey: 11564 spectra with 17.5 (2005)
Le Fevre, O., Vettolani, G., Garilli, B., Tresse, L., Maccagni, D., ...
This paper presents the ``First Epoch\'\' sample from the VIMOS VLT Deep Survey (VVDS). The VVDS goals, observations, data reduction with VIPGI, and redshift measurement with KBRED are discussed....
Le Fevre, O., Guzzo, L., Meneux, B., Pollo, A., Cappi, A., Colombi, S., ...
This paper presents the evolution of the clustering of the main population of galaxies from z=2.1 to z=0.2, from the first epoch VIMOS VLT Deep Survey (VVDS), a magnitude limited sample with 17.5
Ilbert, O., Tresse, L., Zucca, E., Bardelli, S., Arnouts, S., Zamorani, G., ...
We investigate the evolution of the galaxy luminosity function from the VIMOS-VLT Deep Survey (VVDS) from the present to z=2 in five (U, B, V, R and I) rest-frame band-passes. We use the first epoch...
The VIMOS Integral Field Unit: data reduction methods and quality assessment (2005)
Zanichelli, A., Garilli, B., Scodeggio, M., Franzetti, P., Rizzo, D., Maccagni, D., ...
With new generation spectrographs integral field spectroscopy is becoming a widely used observational technique. The Integral Field Unit of the VIsible Multi-Object Spectrograph on the ESO-VLT allows...
The VIRMOS deep imaging survey IV: Near-infrared observations (2005)
Iovino, A., McCracken, H. J., Garilli, B., Foucaud, S., Fevre, O. Le, Maccagni, D., ...
In this paper we present a new deep, wide-field near-infrared imaging survey. Our J- and K-band observations in four separate fields complement optical BVRI, ultraviolet and spectroscopic...
The VIMOS VLT Deep Survey: Evolution of the non-linear galaxy bias up to z=1.5 (2005)
Marinoni, C., Fevre, O. Le, Meneux, B., Iovino, A., Pollo, A., Ilbert, O., ...
We present the first measurements of the Probability Distribution Function (PDF) of galaxy fluctuations in the VIMOS-VLT Deep Survey (VVDS) cone, covering 0.4x0.4 deg between 0.4
Ciliegi, P., Zamorani, G., Bondi, M., Pozzetti, L., Bolzonella, M., Gregorini, L., ...
In this paper we present the optical and near-infrared identifications of the 1054 radio sources detected in the 20cm deep radio survey down to a 5sigma flux limit of about 80 microJy obtained with...
The masses of X-ray emitting EROs (2005)
Brusa, M., Comastri, A., Daddi, E., Pozzetti, L., Zamorani, G., Vignali, C., ...
The VVDS: early results on the large scale structure distribution of galaxies out to z ~ 1.5 (2005)
Le Fevre, O., Vettolani, G., Maccagni, D., Picat, J. P., Adami, C., Arnaboldi, M., ...
The very large telescope visible multi-object spectrograph mask preparation software (2005)
Bottini, D., Garilli, B., Maccagni, D., Tresse, L., Le Brun, V., Le Fevre, O., ...
Pollo, A., Meneux, B., Guzzo, L., Le Fèvre, O., Blaizot, J., Cappi, A., ...
Le Fèvre, O., Guzzo, L., Meneux, B., Pollo, A., Cappi, A., Colombi, S., ...
A large population of galaxies 9 to 12 billion years back in the history of the universe (2005)
Le Fèvre, O., Paltani, S., Arnouts, S., Charlot, S., Foucaud, S., Ilbert, O., ...
The VIRMOS deep imaging survey - IV. Near-infrared observations (2005)
Iovino, A., McCracken, H. J., Garilli, B., Foucaud, S., Le Fèvre, O., Maccagni, D., ...
The VIMOS integral field unit: data-reduction methods and quality assessment (2005)
Zanichelli, A., Garilli, B., Scodeggio, M., Franzetti, P., Rizzo, D., Maccagni, D., ...
The VIMOS VLT deep survey: evolution of the non-linear galaxy bias up to z = 1.5 (2005)
Marinoni, C., Le Fèvre, O., Meneux, B., Iovino, A., Pollo, A., Ilbert, O., ...
Early results from the VIMOS VLT deep survey (2005)
Le Fèvre, O., Adami, C., Ilbert, O., Le Brun, V., Marinoni, C., Mazure, A., ...
The B-Band Luminosity Function of Red and Blue Galaxies up to z=3.5 (2004)
Giallongo, E., Salimbeni, S., Menci, N., Zamorani, G., Fontana, A., Dickinson, M., ...
We have explored the redshift evolution of the luminosity function of red and blue galaxies up to $z=3.5$. This was possible joining a deep I band composite galaxy sample, which includes the...
Schiminovich, D., Ilbert, O., Arnouts, S., Milliard, B., Tresse, L., Fevre, O. Le, ...
In a companion paper (Arnouts et al. 2004) we presented new measurements of the galaxy luminosity function at 1500 Angstroms out to z~1 using GALEX-VVDS observations (1039 galaxies with NUV0.2) and...
Gilli, R., Daddi, E., Zamorani, G., Tozzi, P., Borgani, S., Bergeron, J., ...
We investigate the spatial clustering of X-ray selected sources in the two deepest X-ray fields to date, namely the 2Msec Chandra Deep Field North (CDFN) and the 1Msec Chandra Deep Field South...
Scodeggio, M., Franzetti, P., Garilli, B., Zanichelli, A., Paltani, S., Maccagni, D., ...
The VIMOS VLT Deep Survey (VVDS), designed to measure 150,000 galaxy redshifts, requires a dedicated data reduction and analysis pipeline to process in a timely fashion the large amount of...
The VLT-VIMOS Mask Preparation Software (2004)
Bottini, D., Garilli, B., Maccagni, D., Tresse, L., Brun, V. Le, Fevre, O. Le, ...
VIMOS (VIsible Multi-Object Spectrograph) is a multi-object imaging spectrograph installed at the VLT (Very large Telescope) at the ESO (European Southern Observatory) Paranal Observatory, especially...
Brusa, M., Comastri, A., Daddi, E., Pozzetti, L., Zamorani, G., Vignali, C., ...
We present the results of a deep (about 80 ks) XMM-Newton survey of the largest sample of near-infrared selected Extremely Red Objects (R-K>5) available to date to K_S< 19.2. At the relatively bright...
The VIMOS VLT Deep Survey - First epoch VVDS-Deep survey: 11564 spectra with 17.5 (2004)
Fevre, O. Le, Vettolani, G., Garilli, B., Tresse, L., Maccagni, D., ...
This paper presents the ``First Epoch'' sample from the VIMOS VLT Deep Survey (VVDS). The VVDS goals, observations, data reduction with VIPGI, and redshift measurement with KBRED are discussed. Data...
Ilbert, O., Tresse, L., Zucca, E., Bardelli, S., Arnouts, S., Zamorani, G., ...
We investigate the evolution of the galaxy luminosity function from the VIMOS-VLT Deep Survey (VVDS) from the present to z=2 in five (U, B, V, R and I) rest-frame band-passes. We use the first epoch...
Fevre, O. Le, Guzzo, L., Meneux, B., Pollo, A., Cappi, A., Colombi, S., ...
This paper presents the evolution of the clustering of the main population of galaxies from z=2.1 to z=0.2, from the first epoch VIMOS VLT Deep Survey (VVDS), a magnitude limited sample with 17.5
Pollo, A., Meneux, B., Guzzo, L., Fevre, O. Le, Blaizot, J., Cappi, A., ...
We are presenting in this paper a detailed account of the methods used to compute the three-dimensional two-point galaxy correlation function in the VIMOS-VLT deep survey (VVDS). We investigate how...
Daddi, E., Cimatti, A., Renzini, A., Fontana, A., Mignoli, M., Pozzetti, L., ...
A simple two color selection based on B-, z-, and K- band photometry is proposed for culling galaxies at 1.41.4, independently on their dust reddening. Instead, objects with BzK2.5 (AB) colors...
Old Galaxies in the Young Universe (2004)
Cimatti, A., Daddi, E., Renzini, A., Cassata, P., Vanzella, E., Pozzetti, L., ...
More than half of all stars in the local Universe are found in massive spheroidal galaxies, which are characterized by old stellar populations with little or no current star formation. In present...
Pozzi, F., Gruppioni, C., Oliver, S., Matute, I., La Franca, F., Lari, C., ...
We present the first determination of the 15 mum luminosity function of galaxies from the European Large Area ISO Survey (ELAIS) southern fields. We have adopted a new criterion to separate the...
The Nature of the Mid-Infrared Population from Optical Identifications of the ELAIS-S1 Sample (2004)
La Franca, F., Gruppioni, C., Matute, I., Pozzi, F., Lari, C., Mignoli, M., ...
We present a multiwavelength catalog (15 mum, R-band, K-band, and 1.4 GHz flux) plus spectroscopic identifications for 406 15 mum sources detected in the European Large Area ISO Survey (ELAIS) region...
The K20 survey. VI. The Distribution of the Stellar Masses in Galaxies up to z~2 (2004)
Fontana, A., Pozzetti, L., Donnarumma, I., Renzini, A., Cimatti, A., Zamorani, G., ...
We present a detailed analysis of the stellar mass content of galaxies up to z=2.5 in the K20 galaxy sample, that has a 92% spectroscopic completeness and a complete $UBVRIzJK_s$ multicolor coverage....
Metal enrichment in near-IR luminous galaxies at z~2: signatures of proto-ellipticals? (2004)
De Mello, Duilia, Daddi, E., Renzini, A., Cimatti, A., Alighieri, S. Di Serego, Pozzetti, L., ...
We present the analysis of the coadded rest-frame UV spectrum (1200
The VIMOS VLT Deep Survey: Public release of 1599 redshifts to IAB (2004)
Fevre, O. Le, Vettolani, G., Paltani, S., Tresse, L., Zamorani, G., Brun, V. Le, ...
{This paper presents the VIMOS VLT Deep Survey around the Chandra Deep Field South (CDFS). We have measured 1599 new redshifts with VIMOS on the European Observatory Very Large Telescope - UT3, in an...
The Mid-IR luminosity function of galaxies in the ELAIS Southern fields (2004)
Pozzi, F., Gruppioni, C., Oliver, S., Matute, I., La Franca, F., Lari, C., ...
We present the first determination of the 15micron luminosity functio galaxies from the European Large Area ISO survey (ELAIS) southern fields. We have adopted a new criterion to separate the...
The nature of the mid-infrared population from optical identifications of the ELAIS-S1 sample (2004)
La Franca, F., Gruppioni, C., Matute, I., Pozzi, F., Lari, C., Mignoli, M., ...
We present a multi-wavelength catalog (15 um, R, K-band, 1.4 GHz flux) plus spectroscopic identifications for 406 15 um sources detected in the ELAIS region S1, over the flux density range 0.5
Bias in the Estimation of Global Luminosity Functions (2004)
Ilbert, O., Tresse, L., Arnouts, S., Zucca, E., Bardelli, S., Zamorani, G., ...
We discuss a bias present in the calculation of the global luminosity function (LF) which occurs when analysing faint galaxy samples. This effect exists because of the different spectral energy...
Scodeggio, M., Franzetti, P., Garilli, B., Zanichelli, A., Paltani, S., Maccagni, D., ...
The VIMOS VLT Deep Survey (VVDS), designed to measure 150,000 galaxy redshifts, requires a dedicated data reduction and analysis pipeline to process in a timely fashion the large amount of...
Schiminovich, D., Ilbert, O., Arnouts, S., Milliard, B., Tresse, L., Fevre, O. Le, ...
In a companion paper (Arnouts et al. 2004) we presented new measurements of the galaxy luminosity function at 1500 Angstroms out to z~1 using GALEX-VVDS observations (1039 galaxies with NUV0.2) and...
Bias in the Estimation of Global Luminosity Functions (2004)
Ilbert, O., Tresse, L., Arnouts, S., Zucca, E., Bardelli, S., Zamorani, G., ...
We discuss a bias present in the calculation of the global luminosity function (LF) which occurs when analysing faint galaxy samples. This effect exists because of the different spectral energy...
The VIMOS VLT Deep Survey: Public release of 1599 redshifts to IAB (2004)
Fevre, O. Le, Vettolani, G., Paltani, S., Tresse, L., Zamorani, G., Brun, V. Le, ...
{This paper presents the VIMOS VLT Deep Survey around the Chandra Deep Field South (CDFS). We have measured 1599 new redshifts with VIMOS on the European Observatory Very Large Telescope - UT3, in an...
The VIMOS VLT Deep Survey: Public release of 1599 redshifts to IAB (2004)
Fevre, O. Le, Vettolani, G., Paltani, S., Tresse, L., Zamorani, G., Brun, V. Le, ...
{This paper presents the VIMOS VLT Deep Survey around the Chandra Deep Field South (CDFS). We have measured 1599 new redshifts with VIMOS on the European Observatory Very Large Telescope - UT3, in an...
Scodeggio, M., Franzetti, P., Garilli, B., Zanichelli, A., Paltani, S., Maccagni, D., ...
The VIMOS VLT Deep Survey (VVDS), designed to measure 150,000 galaxy redshifts, requires a dedicated data reduction and analysis pipeline to process in a timely fashion the large amount of...
Schiminovich, D., Ilbert, O., Arnouts, S., Milliard, B., Tresse, L., Fevre, O. Le, ...
In a companion paper (Arnouts et al. 2004) we presented new measurements of the galaxy luminosity function at 1500 Angstroms out to z~1 using GALEX-VVDS observations (1039 galaxies with NUV0.2) and...
Bias in the Estimation of Global Luminosity Functions (2004)
Ilbert, O., Tresse, L., Arnouts, S., Zucca, E., Bardelli, S., Zamorani, G., ...
We discuss a bias present in the calculation of the global luminosity function (LF) which occurs when analysing faint galaxy samples. This effect exists because of the different spectral energy...
Deep redshift surveys : The VIMOS VLT deep surveys (2004)
Le Fevre, O., Maccagni, D., Picat, J. P., Adami, C., Arnoboldi, M., ...
The nature of the mid-infrared population from optical identifications of the ELAIS-S1 sample (2004)
La Franca, F., Gruppioni, C., Matute, I., Pozzi, F., Lari, C., Mignoli, M., ...
Photometric Redshifts for galaxies in the GOODS southern field (2004)
Mobasher, B., Idzi, R., Benítez, N., Cimatti, A., Christiani, S., Daddi, E., ...
The VIRMOS deep imaging survey: III. ESO/WFI deep U-band imaging of the 0226-04 deep field (2003)
Radovich, M., Arnaboldi, M., Ripepi, V., Massarotti, M., McCracken, H. J., Mellier, Y., ...
In this paper we describe the U-band imaging of the F02 deep field, one of the fields in the VIRMOS Deep Imaging Survey. The observations were done at the ESO/MPG 2.2m telescope at La Silla (Chile)...
Early results from the VIMOS VLT Deep Survey (2003)
Fèvre, O. Le, Vettolani, G., Maccagni, D., Picat, J. P., Adami, C., Arnaboldi, M., ...
The VIMOS VLT Deep Survey (VVDS) is underway to study the evolution of galaxies, large scale structures and AGNs, from the measurement of more than 100000 spectra of faint objects. We present here...
Clues on galaxy and cluster formation from their scaling relations (2003)
Lanzoni, B., Ciotti, L., Cappi, A., Tormen, G., Zamorani, G.
By means of high-resolution N-body simulations in a LambdaCDM cosmology, we verify that scaling relations similar to those observed for nearby galaxy clusters are also defined by their dark matter...
The manifold spectra and morphologies of EROs (2003)
Cimatti, A., Daddi, E., Cassata, P., Pignatelli, E., Fasano, G., Vernet, J., ...
Deep VLT optical spectroscopy, HST+ACS (GOODS) imaging and VLA observations are used to unveil the nature of a complete sample of 47 EROs with R-Ks>5 and Ks
Photometric Redshifts for Galaxies in the GOODS Southern Field (2003)
Mobasher, B., Idzi, R., Benitez, N., Cimatti, A., Cristiani, S., Daddi, E., ...
We use extensive multi-wavelength photometric data from the Great Observatories Origins Deep Survey (GOODS) to estimate photometric redshifts for a sample of 434 galaxies with spectroscopic redshifts...
Near-IR bright galaxies at z~2. Entering the spheroid formation epoch ? (2003)
Daddi, E., Cimatti, A., Renzini, A., Vernet, J., Conselice, C., Pozzetti, L., ...
Spectroscopic redshifts have been measured for 9 K-band luminous galaxies at 1.7 < z < 2.3, selected with Ks < 20 in the "K20 survey" region of the Great Observatories Origins Deep Survey area. Star...
The scaling relations of galaxy clusters and their dark matter halos (2003)
Lanzoni, B., Ciotti, L., Cappi, A., Tormen, G., Zamorani, G.
Like early-type galaxies, also nearby galaxy clusters define a Fundamental Plane, a luminosity-radius, and a luminosity-velocity dispersion relations, whose physical origin is still unclear. By means...
The evolution of the galaxy luminosity function in the rest frame blue band up to z=3.5 (2003)
Poli, F., Giallongo, E., Fontana, A., Menci, N., Zamorani, G., Nonino, M., ...
We present an estimate of the cosmological evolution of the field galaxy luminosity function (LF) in the rest frame 4400 Angstrom B -band up to redshift z=3.5. To this purpose, we use a composite...
The VIRMOS deep imaging survey II: CFH12K BVRI optical data for the 0226-04 deep field (2003)
McCracken, H. J., Radovich, M., Bertin, E., Mellier, Y., Dantel-Fort, M., LeFevre, O., ...
(abridged) In this paper we describe in detail the reduction, preparation and reliability of the photometric catalogues which comprise the 1.2 deg^2 CFH12K-VIRMOS deep field. The survey reaches a...
On the nature of the ISO-selected sources in the ELAIS S2 region (2003)
Pozzi, F., Ciliegi, P., Gruppioni, C., Lari, C., Heraudeau, P., Mignoli, M., ...
We have studied the optical, near-IR and radio properties of a complete sample of 43 sources detected at 15-micron in one of the deeper ELAIS repeatedly observed region. The extragalactic objects in...
Tracing the large scale structure in the Chandra Deep Field South (2003)
Gilli, R., Cimatti, A., Daddi, E., Hasinger, G., Rosati, P., Szokoly, G., ...
We report the discovery of large scale structures of X-ray sources in the 1Msec observation of the Chandra Deep Field South. Two main structures appear as narrow (Delta_z < 0.02) spikes in the source...
The VLA-VIRMOS Deep Field I. Radio observations probing the microJy source population (2003)
Ciliegi, M. Bondi. P., Zamorani, G., Gregorini, L., Vettolani, G., Parma, P., De Ruiter, H., ...
We have conducted a deep survey (r.m.s noise 17 microJy) with the Very Large Array (VLA) at 1.4 GHz, with a resolution of 6 arcsec, of a 1 square degree region included in the VIRMOS VLT Deep Survey....
Cappi, M., Di Cocco, G., Panessa, F., Bassani, L., Caroli, E., Dadina, M., ...
An unbiased estimate of the average intrinsic X-ray properties and column density distribution of Seyfert galaxies in the local Universe is crucial to validate unified models of active galactic...
Gruppioni, C., Pozzi, F., Zamorani, G., Ciliegi, P., Lari, C., Calabrese, E., ...
The radio counterparts to the 15-micron sources in the European Large Area ISO Survey southern fields are identified in 1.4-GHz maps down to about 80 microJy. The radio-MIR correlation is...
The K20 survey. V The evolution of the near-IR Luminosity Function (2003)
Pozzetti, L., Cimatti, A., Zamorani, G., Daddi, E., Menci, N., Fontana, A., ...
We present the galaxy rest-frame near-IR Luminosity Function (LF) and its cosmic evolution to z=1.5 based on a spectroscopic survey of a magnitude limited sample of galaxies with Ks
The VLA-VIRMOS Deep Field I. Radio observations probing the microJy source population (2003)
Ciliegi, M. Bondi. P., Zamorani, G., Gregorini, L., Vettolani, G., Parma, P., De Ruiter, H., ...
We have conducted a deep survey (r.m.s noise 17 microJy) with the Very Large Array (VLA) at 1.4 GHz, with a resolution of 6 arcsec, of a 1 square degree region included in the VIRMOS VLT Deep Survey....
The VIRMOS deep imaging survey: III. ESO/WFI deep U-band imaging of the 0226-04 deep field (2003)
Radovich, M., Arnaboldi, M., Ripepi, V., Massarotti, M., McCracken, H. J., Mellier, Y., ...
In this paper we describe the U-band imaging of the F02 deep field, one of the fields in the VIRMOS Deep Imaging Survey. The observations were done at the ESO/MPG 2.2m telescope at La Silla (Chile)...
The VIRMOS deep imaging survey: III. ESO/WFI deep U-band imaging of the 0226-04 deep field (2003)
Radovich, M., Arnaboldi, M., Ripepi, V., Massarotti, M., McCracken, H. J., Mellier, Y., ...
In this paper we describe the U-band imaging of the F02 deep field, one of the fields in the VIRMOS Deep Imaging Survey. The observations were done at the ESO/MPG 2.2m telescope at La Silla (Chile)...
The VLA-VIRMOS Deep Field I. Radio observations probing the microJy source population (2003)
Ciliegi, M. Bondi. P., Zamorani, G., Gregorini, L., Vettolani, G., Parma, P., De Ruiter, H., ...
We have conducted a deep survey (r.m.s noise 17 microJy) with the Very Large Array (VLA) at 1.4 GHz, with a resolution of 6 arcsec, of a 1 square degree region included in the VIRMOS VLT Deep Survey....
A deep VLA survey at 6 cm in the Lockman Hole (2003)
Ciliegi, P., Zamorani, G., Hasinger, G., Lehmann, I., Szokoly, G., Wilson, G.
We have obtained a deep radio image with the Very Large Array at 6 cm in the Lockman Hole. The noise level in the central part of the field is similar to11 muJy. From these data we have extracted a...
Optical identifications in the Marano field XMM-Newton survey (2003)
Lamer, G., Wagner, S., Zamorani, G., Mignoli, M., Hasinger, G., Giedke, K., ...
Tracing the large-scale structure in the Chandra deep field south. (2003)
Gilli, R., Cimatti, A., Daddi, E., Hasinger, G., Rosati, P., Szokoly, G., ...
A deep VLA survey at 6 cm in the Lockman Hole (2002)
Ciliegi, P., Zamorani, G., Hasinger, G., Lehmann, I., Szokoly, G. P., Wilson, G.
We have obtained a deep radio image with the Very Large Array at 6 cm in the Lockman Hole. The noise level in the central part of the field is about 11 microJy. From these data we have extracted a...
Lari, C., Gruppioni, C., Pozzi, F., Zamorani, G., Franceschini, A., Oliver, S., ...
We present the 15-mum extragalactic source counts from the Final Analysis Catalogue of the European Large Area ISO Survey (ELAIS) Southern hemisphere field S1, extracted using the Lari method. The...
The K20 survey. IV. The redshift distribution of Ks (2002)
Cimatti, A., Pozzetti, L., Mignoli, M., Daddi, E., Menci, N., Poli, F., ...
We present the redshift distribution of a complete sample of 480 galaxies with Ks1 and z>1.5 respectively. A ``blind'' comparison is made with the predictions of a set of the most recent LambdaCDM...
The K20 survey. III. Photometric and spectroscopic properties of the sample (2002)
Cimatti, A., Mignoli, M., Daddi, E., Pozzetti, L., Fontana, A., Saracco, P., ...
The K20 survey is an ESO VLT optical and near-infrared spectroscopic survey aimed at obtaining spectral information and redshifts of a complete sample of about 550 objects to K_s\leq20.0 over two...
Gruppioni, C., Lari, C., Pozzi, F., Zamorani, G., Franceschini, A., Oliver, S., ...
We present the 15 micron extragalactic source counts from the Final Analysis Catalogue of the European Large Area ISO Survey southern hemisphere field S1, extracted using the Lari method. The large...
Matute, I., La Franca, F., Pozzi, F., Gruppioni, C., Lari, C., Zamorani, G., ...
We present the 15-mum luminosity function of type 1 active galactic nuclei (AGN1; quasi-stellar object+Seyfert 1) . Our sample of 21 high-redshift sources is selected from the Preliminary Analysis...
The Evolution of type 1 AGN in the IR (15mu). The view from ELAIS-S1 (2002)
Matute, I., La Franca, F., Pozzi, F., Gruppioni, C., Lari, C., Zamorani, G., ...
We present the 15 micron luminosity function of type 1 AGN (QSO + Seyfert 1). Our sample of 21 high-redshift sources is selected from the Preliminary Analysis catalogue in the S1 field of the...
First Results from a XMM-Newton Survey of a Distance-Limited (D (2002)
Cappi, M., Di Cocco, G., Panessa, F., Foschini, L., Trifoglio, M., Gianotti, F., ...
We report here preliminary results from a survey of nearby Seyfert galaxies using the EPIC CCDs on board XMM-Newton. The total sample consists of 28 Seyfert galaxies, and constitute a well-defined,...
The K20 survey. II. The Different Spatial Clustering of z~1 Old and Dusty Star-Forming EROs (2002)
Daddi, E., Cimatti, A., Broadhurst, T., Renzini, A., Zamorani, G., Mignoli, M., ...
We compare the 3D clustering of old passively-evolving and dusty star-forming z~1 EROs from the K20 survey. With detailed simulations of clustering, the comoving correlation length of dusty...
Most Supermassive Black Holes must be Rapidly Rotating (2001)
Elvis, M., Risaliti, G., Zamorani, G.
We use the integrated spectrum of the X-ray background and quasars Spectral Energy Distribution to derive the contribution of quasars to the energy output of the Universe. We find a lower limit for...
The K20 survey. I. Disentangling old and dusty star-forming galaxies in the ERO population (2001)
Cimatti, A., Daddi, E., Mignoli, M., Pozzetti, L., Renzini, A., Zamorani, G., ...
We present the results of VLT optical spectroscopy of a complete sample of 78 EROs with R-Ks\geq5 over a field of 52 arcmin^2. About 70% of the 45 EROs with Ks\leq19.2 have been spectroscopically...
Radio-optically selected clusters of galaxies. II. The cluster sample (2001)
Zanichelli, A., Scaramella, R., Vettolani, G., Vigotti, M., Bardelli, S., Zamorani, G.
We present a sample of 171 candidate groups and clusters of galaxies at intermediate redshift over an area of ~550 square degrees at the South Galactic Pole selected by using optically identified...
The Spatial Clustering of Distant, z~1, Early-Type Galaxies (2001)
Daddi, E., Broadhurst, T., Zamorani, G., Cimatti, A., Rottgering, H., Renzini, A.
We examine the spatial clustering of extremely red objects (EROs) found in a relatively large survey of 700 arcmin^2, containing 400 galaxies with R-Ks>5 to Ks=19.2. A comoving correlation length...
The ROSAT Deep Survey: VI. X-ray sources and Optical identifications of the Ultra Deep Survey (2001)
Lehmann, I., Hasinger, G., Schmidt, M., Giacconi, R., Truemper, J., Zamorani, G., ...
We describe in this paper the ROSAT Ultra Deep Survey (UDS), an extension of the ROSAT Deep Survey (RDS) in the Lockman Hole. The UDS reaches a flux level of 1.2 x 10E-15 erg/cm2/s in 0.5-2.0 keV...
The VIRMOS-VLT Deep Survey (2001)
Fèvre, O. Le, Vettolani, G., Maccagni, D., Mancini, D., Mazure, A., Mellier, Y., ...
The aim of the VIRMOS VLT Deep Survey (VVDS) is to study of the evolution of galaxies, large scale structures and AGNs from a sample of more than 150,000 galaxies with measured redshifts in the range...
The spatial clustering of distant, z ~ 1, early-type galaxies (2001)
Daddi, E., Broadhurst, T., Zamorani, G., Cimatti, A., Röttgering, H., Renzini, A.
The spatial clustering of distant, z ~ 1, early-type galaxies (2001)
Daddi, E., Broadhurst, T., Zamorani, G., Cimatti, A., Röttgering, H.J.A., Renzini, A.
Large-scale distribution and spectral properties of galaxies in the Shapley Concentration (2000)
Zucca, E., Bardelli, S., Baldi, A., Zamorani, G., Moscardini, L., Scaramella, R.
We present the results of a redshift survey of both cluster and intercluster galaxies in the central part of the Shapley Concentration, the richest supercluster of clusters in the nearby Universe,...
The violent environment of the Shapley Concentration: a multiwavelength view (2000)
Bardelli, S., Zucca, E., Venturi, T., Morganti, R., Hunstead, R. W., Ettori, S., ...
Rich superclusters are the ideal environment for the detection of cluster mergings, because the high peculiar velocities induced by the enhanced local density of the large-scale structure favour the...
BeppoSAX - ROSAT PSPC observations of the Shapley Supercluster: A3562 (2000)
Ettori, S., Bardelli, S., De Grandi, S., Molendi, S., Zamorani, G., Zucca, E.
We present a combined analysis of the BeppoSAX and ROSAT PSPC observation of the cluster of galaxies A3562, a massive member of the core of the Shapley Supercluster. With a complex and interacting...
Daddi, E., Cimatti, A., Pozzetti, L., Hoekstra, H., Röttgering, H. J. A., Renzini, A., ...
We present the results of a wide-field survey for extremely red objects (EROs hereafter), the widest so far, based on Ks and R band imaging. The survey covers 701 arcmin^2 and it is 85% complete to...
The contribution of Narrow-Line Seyfert 1 galaxies to the soft X-ray background (2000)
Hasinger, G., Lehmann, I., Schmidt, M., Gunn, J. E., Schneider, D. P., Giacconi, R., ...
The ROSAT Ultradeep HRI survey in the Lockman Hole contains a complete sample of 91 X-ray sources with fluxes in the 0.5-2 keV band larger than 1.2 times 10e-15 erg cm-2 s-1, where over about 75 per...
The ROSAT Deep Survey: III. Optical spectral properties of X-ray sources in the Lockman Hole (1999)
Lehmann, I., Hasinger, G., Schmidt, M., Gunn, J. E., Schneider, D. P., Giacconi, R., ...
The ROSAT Deep Survey in the Lockman Hole contains a complete sample of 50 X-ray sources with fluxes in the 0.5-2.0 keV band larger than 5.5E-15 erg/cm2/s. Previous work has provided optical...
New Clues on the Nature of Extremely Red Galaxies (1999)
Cimatti, A., Daddi, E., Alighieri, S. Di Serego, Pozzetti, L., Mannucci, F., Renzini, A., ...
We present near-infrared VLT-UT1+ISAAC spectroscopy of a sample of 9 extremely red galaxies (ERGs) with R-K>5 and K
Bardelli, S., Zucca, E., Zamorani, G., Moscardini, L., Scaramella, R.
(abridged) We present the results of a redshift survey of intercluster galaxies in the central region of the Shapley Concentration supercluster, aimed at determining the distribution of galaxies in...
The X-Ray Luminosity Function of Active Galactic Nuclei (1999)
Schmidt, M., Giacconi, R., Hasinger, G., Truemper, J., Zamorani, G.
We derive an X-ray luminosity function for active galactic nuclei (AGN) that accounts for the X-ray source counts in the 0.5-2.0 and 2-10 keV energy ranges, the redshift distribution of AGNs in the...
The ROSAT deep survey: V. X-rays Sources and Optical Identifications in the Marano Field (1999)
Zamorani, G., Mignoli, M., Hasinger, G., Burg, R., Giacconi, R., Schmidt, M., ...
We present the X-ray data and the optical identifications for a deep ROSAT PSPC observation in the "Marano field". In the inner region of the ROSAT field (15' radius) we detected 50 X-ray sources...
Guzzo, L., Bartlett, J. G., Cappi, A., Maurogordato, S., Zucca, E., Zamorani, G., ...
We present analyses of the two-point correlation properties of the ESP galaxy redshift survey. From the redshift-space correlation function xi(s), we see positive clustering out to separations ~50/h...
Hasinger, G., Lehmann, I., Giacconi, R., Schmidt, M., Truemper, J., Zamorani, G.
The ROSAT Deep Survey in the Lockman Hole is the most sensitive X-ray survey performed to date, encompassing an exposure time of 200 ksec with the PSPC and 1.2 Msec with the HRI. The source counts...
New clues on the nature of extremely red galaxies (1999)
Cimatti, A., Daddi, E., Serego Alighieri, S. Di, Pozzetti, L., Mannucci, F., Renzini, A., ...
New clues on the nature of extremely red galaxies (1999)
Cimatti, A., Daddi, E., Serego Alighieri, S. Di, Pozzetti, L., Mannucci, F., Renzini, A., ...
The ESO Slice Project (ESP) galaxy redshift survey: VI Groups of Galaxies (1998)
Ramella, M., Zamorani, G., Zucca, E., Stirpe, G. M., Vettolani, G., Balkowski, C., ...
In this paper we identify objectively and analyze groups of galaxies in the recently completed ESP survey. We find 231 groups above the number overdensity threshold delta(rho)/rho=80 in the redshift...
Bassani, L., Dadina, M., Maiolino, R., Salvati, M., Risaliti, G., Della Ceca, R., ...
We present and discuss a "3-dimensional" diagnostic diagram for Seyfert2 galaxies obtained by means of X-ray and [OIII] data on a large sample of objects (reported in the Appendix). The diagram shows...
The large-scale distribution of galaxies in the Shapley Concentration (1998)
Bardelli, S., Zucca, E., Zamorani, G.
We present the results of a galaxy redshift survey in the central region of the Shapley Concentration. Our total sample contains ~2000 radial velocities of galaxies both in the clusters and in the...
The ROSAT Deep Survey IV. A distant lensing cluster of galaxies with a bright arc (1998)
Hasinger, G., Giacconi, R., Gunn, J. E., Lehmann, I., Schmidt, M., Schneider, D. P., ...
An unusual double-lobed extended X-ray source (RX J105343+5735) is detected in the ROSAT ultra-deep HRI image of the Lockman Hole. The angular size of the source is 1.7 X 0.7 arcmin^2 and its X-ray...
The Luminosity Function and Mean Galaxy Density from the ESP galaxy Redshift Survey (1998)
Zucca, E., Zamorani, G., Vettolani, P.
We summarise the main results obtained over the last two years by the ESO Slice Project (ESP) redshift survey, concerning the luminosity function and mean density of galaxies, and their implications...
A substructure analysis of the A3558 cluster complex (1998)
Bardelli, S., Pisani, A., Ramella, M., Zucca, E., Zamorani, G.
The "algorithm driven by the density estimate for the identification of clusters" (DEDICA, Pisani 1993, 1996) is applied to the A3558 cluster complex in order to find substructures. This complex,...
Heavy obscuration in X-ray weak AGNs (1998)
Maiolino, R., Salvati, M., Bassani, L., Dadina, M., Della Ceca, R., Matt, G., ...
We present observations in the 0.1-100 keV spectral band of 8 Seyfert 2 galaxies, obtained by means of BeppoSAX. These sources were selected according to their [OIII] optical emission line flux, to...
Cappi, A., Zamorani, G., Zucca, E., Vettolani, G., Merighi, R., Mignoli, M., ...
We present a detailed discussion of the redshift errors associated to the ESO Slice Project measurements. For a subsample of 742 galaxies with redshifts determined both from the absorption lines...
The ESO Slice Project (ESP) galaxy redshift survey: III. The Sample (1998)
Vettolani, G., Zucca, E., Merighi, R., Mignoli, M., Proust, D., Zamorani, G., ...
The ESO Slice Project (ESP) is a galaxy redshift survey extending over about 23 square degrees, in a region near the South Galactic Pole. The survey is ~85% complete to the limiting magnitude...
High Redshift Galaxies in the Hubble Deep Field: II. Colours and Number Counts (1998)
Pozzetti, L., Madau, P., Zamorani, G., Ferguson, H. C., Bruzual, G. A.
We discuss the deep galaxy counts from the Hubble Deep Field (HDF) imaging survey. At faint magnitudes, the slope of the differential number-magnitude relation is flatter than 0.2 in all four HDF...
Scaramella, R., Guzzo, L., Zamorani, G., Zucca, E., Balkowski, C., Blanchard, A., ...
The issue of the approximate isotropy and homogeneity of the observable universe is one of the major topics in modern Cosmology: the common use of the Friedmann-Robertson-Walker [FWR] metric relies...
Bardelli, S., Zucca, E., Zamorani, G., Vettolani, G., Scaramella, R.
The Shapley Concentration is the richest supercluster of clusters in the nearby universe and its core is a remarkable complex formed by the ACO clusters A3558, A3562 and A3556, and by the two minor...
BeppoSAX observations of Narrow-Line Seyfert 1 galaxies:I. Ton S 180 (1997)
Comastri, A., Fiore, F., Guainazzi, M., Matt, G., Stirpe, G. M., Zamorani, G., ...
We report on the first spectrum up to 10 keV of the bright narrow-line Seyfert 1 galaxy Ton S 180, obtained with the imaging instruments onboard BeppoSAX. This is the first observed source in a...
X-ray detections of weak Seyfert2's with BeppoSAX (1997)
Salvati, M., Bassani, L., Della Ceca, R., Maiolino, R., Matt, G., Zamorani, G.
We report the detection in the X rays of two weak Seyfert2's (NGC3393 and NGC4941) with the Italian-Dutch satellite BeppoSAX. These are among the first sources observed in a sample of 12 Seyfert2's...
Zucca, E., Zamorani, G., Vettolani, G., Cappi, A., Merighi, R., Mignoli, M., ...
(Abridged) The ESO Slice Project (ESP) is a galaxy redshift survey we have completed as an ESO Key-Project over ~23 square degrees, in a region near the South Galactic Pole. The survey is nearly...
The ESO Slice Project (ESP) galaxy redshift survey: I. Description and First Results (1997)
Vettolani, G., Zucca, E., Zamorani, G., Cappi, A., Merighi, R., Mignoli, M., ...
The ESO Slice Project (ESP) is a galaxy redshift survey we have recently completed as an ESO Key-Project. The ESP covers 23.3 square degrees in a region close to the South Galactic Pole. The survey...
Pure Luminosity Evolution models for faint field galaxy samples (1996)
Pozzetti, L., A., G. Bruzual, Zamorani, G.
We have examined a set of pure luminosity evolution (PLE) models in order to explore up to what extent the rapidly increasing observational constraints from faint galaxy samples can be understood in...
A study of the core of the Shapley Concentration: II. ROSAT observation of A3558 (1995)
Bardelli, S., Zucca, E., Malizia, A., Zamorani, G., Scaramella, R., Vettolani, G.
We present the results of a pointed ROSAT PSPC observation of the cluster A3558 which is part of the core of the Shapley Concentration. The X-ray brightness distribution can be fitted as the sum of...
Preliminary Results from the ESO Slice Project (ESP) (1994)
Vettolani, G., Zucca, E., Cappi, A., Merighi, R., Mignoli, M., Stirpe, G., ...
We present the first results of a galaxy redshift survey, ESO Slice Project (ESP), we are accomplishing as an ESO Key-Project over about 30 square degrees in a region near the South Galactic Pole....
The contribution of AGNs to the X-ray background (1994)
Comastri, A., Setti, G., Zamorani, G., Hasinger, G.
We report the results of a detailed analysis of the contribution of various classes of AGNs to the extragalactic X-ray background (XRB). The model is based on the unification schemes of AGNs and on...
Preliminary Results from the ESO Slice Project (ESP) (1993)
Vettolani, G., Zucca, E., Cappi, A., Merighi, R., Mignoli, M., Stirpe, G., ...
We present the first results of a galaxy redshift survey, ESO Slice Project (ESP), we are accomplishing as an ESO Key--Project over about 40 square degrees in a region near the South Galactic Pole....
Study of the Core of the Shapley Concentration: I.the Sample (1993)
Bardelli, S., Zucca, E., Vettolani, G., Zamorani, G.
We report the first results of a spectroscopic survey of galaxies in the core of the Shapley Concentration, the richest nearby supercluster of clusters of galaxies. We have measured 311 new galaxy...
Senno, L. Del, Zamorani, G., Piva, R., Hanau, S., Buzzoni, D., ...
A highly polymorphic DNA probe (3′HVR) with genetic linkage to the locus of autosomal dominant polycystic kidney disease was used for screening. Families with subjects at risk were from the Po...