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
The Build-Up of the Hubble Sequence in the COSMOS Field (2009)
Oesch, P. A., Carollo, C. M., Feldmann, R., Hahn, O., Lilly, S. J., Sargent, M. T., ...
We use ~8,600 >5e10 Msol COSMOS galaxies to study how the morphological mix of massive ellipticals, bulge-dominated disks, intermediate-bulge disks, bulge-less disks and irregular galaxies evolves...
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...
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...
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...
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)...
On the nature of red galaxies: the Chandra perspective (2009)
Campisi, M. A., Vignali, C., Brusa, M., Daddi, E., Comastri, A., Pozzetti, L., ...
We present the X-ray properties of the extremely red objects (ERO) population observed by Chandra with three partially overlapping pointings (up to ~90 ks) over an area of ~500 arcmin^2, down to a...
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
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...
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...
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)...
Mannucci, F., Cresci, G., Maiolino, R., Marconi, A., Pastorini, G., Pozzetti, L., ...
We present the first results of a project, LSD, aimed at obtaining spatially-resolved, near-infrared spectroscopy of a complete sample of Lyman-Break Galaxies at z~3. Deep observations with adaptive...
Searching for massive galaxies at z>=3.5 in GOODS-North (2009)
Mancini, C., Matute, I., Cimatti, A., Daddi, E., Dickinson, M., Rodighiero, G., ...
We constrain the space density and properties of massive galaxy candidates at redshifts of z>=3.5 in the GOODS-N field. By selecting sources in the Spitzer+IRAC bands, a highly stellar mass-complete...
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...
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...
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...
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., ...
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., ...
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., ...
On the nature of red galaxies: the Chandra perspective (2009)
Campisi, M. A., Vignali, C., Brusa, M., Daddi, E., Comastri, A., Pozzetti, L., ...
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...
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...
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...
Rodrigues, M., Hammer, F., Flores, H., Puech, M., Liang, Y. C., Fuentes-Carrera, I., ...
Intermediate mass galaxies (logM(Msun)>10) at z~0.6 are the likeliest progenitors of the present-day numerous population of spirals. There is growing evidence that they have evolved rapidly since the...
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...
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
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...
The VIMOS-VLT Deep Survey: Dependence of galaxy clustering on stellar mass (2008)
Meneux, B., Guzzo, L., Garilli, B., Fevre, O. Le, Pollo, A., Blaizot, J., ...
We have investigated the dependence of galaxy clustering on their stellar mass at z~1, using the data from the VIMOS-VLT Deep Survey (VVDS). We have measured the projected two-point correlation...
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...
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...
IMAGES-III: The evolution of the Near-Infrared Tully-Fisher relation over the last 6 Gyr (2008)
Puech, M., Flores, H., Hammer, F., Yang, Y., Neichel, B., Lehnert, M., ...
Using the multi-integral field spectrograph GIRAFFE at VLT, we have derived the K-band Tully-Fisher relation (TFR) at z~0.6 for a representative sample of 65 galaxies with emission lines. We confirm...
Neichel, B., Hammer, F., Puech, M., Flores, H., Lehnert, M., Rawat, A., ...
We present a first combined analysis of the morphological and dynamical properties for the Intermediate MAss Galaxy Evolution Sequence (IMAGES) sample. It is a representative sample of 52 z~0.6...
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., ...
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., ...
Images I. Strong evolution of galaxy kinematics since z=1 (2008)
Yang, Y., Flores, H., Hammer, F., Neichel, B., Puech, M., Nesvadba, N., ...
IMAGES. I. Strong evolution of galaxy kinematics since z = 1 (2008)
Yang, Y., Flores, H., Hammer, F., Neichel, B., Puech, M., Nesvadba, N., ...
Nearly half the stellar mass of present-day spiral galaxies has formed since z = 1, and galaxy kinematics is an ideal tool to identify the underlying mechanisms responsible for the galaxy mass...
Rodrigues, M., Hammer, F., Flores, H., Puech, M., Liang, Y. C., Fuentes-Carrera, I., ...
Context: Intermediate mass galaxies (> 1010 M_o) at z ~ 0.6 are the likeliest progenitors of the present-day, numerous population of spirals. There is growing evidence that they have evolved rapidly...
IMAGES. III. The evolution of the near-infrared Tully-Fisher relation over the last 6 Gyr (2008)
Puech, M., Flores, H., Hammer, F., Yang, Y., Neichel, B., Lehnert, M., ...
Using the multi-integral field spectrograph GIRAFFE at VLT, we have derived the K-band Tully-Fisher relation (TFR) at z ÃÅ 0.6 for a representative sample of 65 galaxies with emission lines...
Neichel, B., Hammer, F., Puech, M., Flores, H., Lehnert, M., Rawat, A., ...
We present a first combined analysis of the morphological and dynamical properties for the intermediate-mass Galaxy Evolution Sequence (IMAGES) sample. It is a representative sample of 52...
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...
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...
IMAGES I. Strong evolution of galaxy kinematics since z=1 (2007)
Yang, Y., Flores, H., Hammer, F., Neichel, B., Puech, M., Nesvadba, N., ...
(abbreviated) We present the first results of the ESO large program, ``IMAGES'' which aims at obtaining robust measurements of the kinematics of distant galaxies using the multi-IFU mode of GIRAFFE...
The HELLAS2XMM survey: XI. Unveiling the nature of X-ray Bright Optically Normal Galaxies (2007)
Civano, F., Mignoli, M., Comastri, A., Vignali, C., Fiore, F., Pozzetti, L., ...
X-ray Bright Optically Normal Galaxies (XBONGs) constitute a small but not negligible fraction of hard X-ray selected sources in recent Chandra and XMM-Newton surveys. Even though several...
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
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)...
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...
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...
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...
Ravikumar, C. D., Puech, M., Flores, H., Proust, D., Hammer, F., Lehnert, M., ...
(Abbrev.) This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequence (IMAGES) up to z=1. Intermediate mass galaxies (MJ
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 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., ...
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., ...
Le Fèvre, O., Arnouts, S., Guzzo, L., Farrah, D., Iovino, A., ...
The HELLAS2XMM survey - XI. Unveiling the nature of X-ray bright optically normal galaxies (2007)
Civano, F., Mignoli, M., Comastri, A., Vignali, C., Fiore, F., Pozzetti, L., ...
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., ...
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., ...
Ravikumar, C. D., Puech, M., Flores, H., Proust, D., Hammer, F., Lehnert, M., ...
Context: .This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequence (IMAGES) up to a redshift of one. Intermediate mass galaxies (MJ
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...
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., ...
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...
Ravikumar, C. D., Puech, M., Flores, H., Proust, D., Hammer, F., Lehnert, M., ...
(Abbrev.) This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequence (IMAGES) up to z=1. Intermediate mass galaxies (MJ
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...
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 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
Evidence for strong evolution of the cosmic star formation density at high redshift (2006)
Mannucci, F., Buttery, H., Maiolino, R., Marconi, A., Pozzetti, L.
Deep HST/ACS and VLT/ISAAC data of the GOODS-South field were used to look for high-redshift galaxies in the rest-frame UV wavelength range and to study the evolution of the cosmic star-formation...
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: 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...
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
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...
The HELLAS2XMM survey: IX. Spectroscopic identification of super-EROs hosting AGNs (2006)
Maiolino, R., Mignoli, M., Pozzetti, L., Severgnini, P., Brusa, M., Vignali, C., ...
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., ...
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
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 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 HELLAS2XMM survey. IX. Spectroscopic identification of super-EROs hosting AGNs (2005)
Maiolino, R., Mignoli, M., Pozzetti, L., Severgnini, P., Brusa, M., Vignali, C., ...
We present VLT near-IR spectroscopic observations of three X-ray sources characterized by extremely high X-ray-to-optical ratios (X/O>40), extremely red colors (6.3
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...
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...
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 Vimos VLT deep survey: compact structures in the CDFS (2005)
Adami, C., Mazure, A., Ilbert, O., Cappi, A., Bottini, D., Garilli, B., ...
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...
Cassata, P., Cimatti, A., Franceschini, A., Daddi, E., Pignatelli, E., Fasano, G., ...
We present a detailed analysis of the evolution of the rest-frame B-band morphology of K-selected galaxies with 0 < z < 2.5. This work is based on the K20 spectroscopic sample (Ks
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...
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 HELLAS2XMM survey. V. Near-Infrared observations of X-ray sources with extreme X/O ratios (2004)
Mignoli, M., Pozzetti, L., Comastri, A., Brusa, M., Ciliegi, P., Cocchia, F., ...
We present the results of deep near-infrared observations of 11 hard X-ray selected sources in the Hellas2XMM survey, with faint optical magnitude (R>24) and high X-ray-to-optical flux ratio. All but...
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...
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
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 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 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 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 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....
Extremely Red Objects: an X-ray dichotomy (2002)
Brusa, M., Comastri, A., Daddi, E., Cimatti, A., Mignoli, M., Pozzetti, L.
We analyze the X-ray properties of a near-infrared selected (Ks < 20) sample of spectroscopically identified Extremely Red Objects (R-Ks>5) in a region of the Chandra Deep Field-South using 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...
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...
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...
The relative abundances of ellipticals and starbursts among the Extremely Red Galaxies (2001)
Mannucci, F., Pozzetti, L., Thompson, D., Oliva, E., Baffa, C., Comoretto, G., ...
We present J band observations of a complete sample of 57 red galaxies selected to have K5.3. We use the Pozzetti and Mannucci (2000) prescriptions, based on the R-K and J-K colours, to separate the...
Mannucci, F., Basile, F., Poggianti, B. M., Cimatti, A., Daddi, E., Pozzetti, L., ...
We have observed 28 local galaxies in the wavelength range between 1 and 2.4 mic in order to define template spectra of the normal galaxies along the Hubble sequence. Five galaxies per morphological...
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...
Extremely red galaxies: age and dust degeneracy solved ? (2000)
The extremely red galaxies (ERGs) are defined in terms of their very red optical-to-near IR colours (as R-K>5 or I-K>4). Originally this selection was aimed at selecting old (> 1 Gyr) passively...
The density of extremely red objects around high-z radio-loud AGN (2000)
Cimatti, A., Villani, D., Pozzetti, L., Alighieri, S. Di Serego
We present the results of a K-band imaging survey of 40 arcmin^{2} in fields around 14 radio-loud AGN (6 radio galaxies and 8 quasars) with z>1.5. The survey, 80% complete to K1.5 radio galaxies and...
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...
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
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., ...
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...
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...
The genetic and non-genetic toxicity of the fungicide Vinclozolin (1996)
Hrelia, P., Fimognari, C., Maffei, F., Vigagni, F., Mesirca, R., Pozzetti, L., ...
The mutagenic/cocarcinogenic, potential of the fungicide Vinclozolin was assessed by a comprehensive examinationof toxicity mechanisms at both the genetic and the metabolic level. Vinclozolin did...
Paolini, M., Mesirca, R., Pozzetti, L., Silingardi, P., Grilli, S., Cantelli-Forti, G.
The aim of this work was to optimize the ionic strength (τ) in the liver microsomal assay (LMA) hi performing short-term genotoxicity tests, τ optimization would increase the sensitivity (i.e....