The Opacity of Galactic Disks at z~0.7 (2010)
Sargent, Mark T., Carollo, C. M., Kampczyk, P., Lilly, S. J., Scarlata, C., Capak, P., ...
We compare the surface brightness-inclination relation for a sample of COSMOS pure disk galaxies at z~0.7 with an artificially redshifted sample of SDSS disks well matched to the COSMOS sample in...
Cassata, P., Fevre, O. Le, Garilli, B., Maccagni, D., Brun, V. Le, Scodeggio, M., ...
Aims. The aim of this work is to study the contribution of the Ly-alpha emitters to the Star Formation Rate Density (SFRD) of the Universe in the interval 2 < z < 6.6. Methods. We have assembled a...
Ultraluminous X-ray sources out to z~0.3 in the COSMOS field (2010)
Mainieri, V., Vignali, C., Merloni, A., Civano, F., Puccetti, S., Brusa, M., ...
Using Chandra observations we have identified a sample of seven off-nuclear X-ray sources, in the redshift range z=0.072-0.283, located within optically bright galaxies in the COSMOS Survey. Using...
Kartaltepe, Jeyhan S., Sanders, D. B., Le Floc'h, E., Frayer, D. T., Aussel, H., Arnouts, S., ...
We present a large robust sample of 1503 reliable and unconfused 70 μm selected sources from the multiwavelength data set of the Cosmic Evolution Survey. Using the Spitzer IRAC and MIPS photometry,...
Galaxy Stellar Mass Assembly Between 0.2 < z < 2 from the S-COSMOS Survey (2010)
Ilbert, O., Salvato, M., Le Floc'h, E., 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...
Sargent, M. T., Schinnerer, E., Murphy, E., Aussel, H., Le Floc'h, E., Frayer, D. T., ...
VLA 1.4 GHz (σ ~ 0.012 mJy) and MIPS 24 and 70 μm (σ ~ 0.02 and 1.7 mJy, respectively) observations covering the 2 deg^2 COSMOS field are combined with an extensive multiwavelength data set to...
Sargent, Mark T., Schinnerer, E., Murphy, E., Aussel, H., Floc'h, E. Le, Frayer, D. T., ...
VLA 1.4 GHz (rms noise ~0.012 mJy) and MIPS 24 and 70 micron (rms noise ~0.02 and ~1.7 mJy, respectively) observations covering the 2 square degree COSMOS field are combined with an extensive...
Bars in early- and late-type disks in COSMOS (2010)
Cameron, E., Carollo, C. M., Oesch, P., Aller, M. C., Bschorr, T., Cerulo, P., ...
We investigate the bar fraction in a mass-complete sample of M > 10^10.5 Msun disk galaxies at 0.2 < z < 0.6 in the COSMOS field. The fraction of barred disks strongly depends on mass, disk...
McCracken, H. J., Capak, P., Salvato, M., Aussel, H., Thompson, D., Daddi, E., ...
We present a new near-infrared survey covering the 2 deg^2 COSMOS field conducted using WIRCam at the Canada-France-Hawaii Telescope. By combining our near-infrared data with Subaru B and z images,...
Goto, Tomotsugu, Takagi, T., Matsuhara, H., Takeuchi, T. T., Pearson, C., Wada, T., ...
Dust-obscured star-formation becomes much more important with increasing intensity, and increasing redshift. We aim to reveal cosmic star-formation history obscured by dust using deep infrared...
Drory, N., Bundy, K., Leauthaud, A., Scoville, N., Capak, P., Ilbert, O., ...
We present a new analysis of stellar mass functions in the COSMOS field to fainter limits than has been previously probed at z ≤ 1. The increase in dynamic range reveals features in the shape of...
Caputi, K. I., Lilly, S. J., Aussel, H., Le Floc'h, E., Sanders, D., Maier, C., ...
We have used the zCOSMOS-bright 10k sample to identify 3244 Spitzer/MIPS 24 μm-selected galaxies with 0.06 mJy < S_(24 μm) ≾ 0.50 mJy and I_(AB) < 22.5, over 1.5 deg^2 of the COSMOS field, and...
Bundy, K., Scarlata, C., Carollo, C. M., Ellis, R. S., Drory, N., Hopkins, P., ...
The increasing abundance of passive "red sequence" galaxies since z=1-2 is mirrored by a coincident rise in the number of galaxies with spheroidal morphologies. In this paper, however, we show that...
Zucca, E., Bardelli, S., Bolzonella, M., Zamorani, G., Ilbert, O., Pozzetti, L., ...
Aims. An unbiased and detailed characterization of the galaxy luminosity function (LF) is a basic requirement in many astrophysical issues: it is of particular interest in assessing the role of the...
Kartaltepe, Jeyhan S., Sanders, D. B., Floc'h, E. Le, Frayer, D. T., Aussel, H., Arnouts, S., ...
We present a large robust sample of 1503 reliable and unconfused 70microm selected sources from the multiwavelength data set of the Cosmic Evolution Survey (COSMOS). Using the Spitzer IRAC and MIPS...
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 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...
Spitzer 70 and 160 μm Observations of the COSMOS Field (2009)
Frayer, D. T., Sanders, D. B., Surace, J. A., Aussel, H., Salvato, M., Le Floc'h, E., ...
We present Spitzer 70 and 160 μm observations of the COSMOS Spitzer survey (S-COSMOS). The data processing techniques are discussed for the publicly released products consisting of images and source...
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...
Drory, N., Bundy, K., Leauthaud, A., Scoville, N., Capak, P., Ilbert, O., ...
We present a new analysis of stellar mass functions (MF) in the COSMOS field to fainter limits than has been previously probed to z~1. Neither the total nor the passive or star-forming MF can be well...
Leauthaud, A., Finoguenov, A., Kneib, J. P., Taylor, J. E., Massey, R., Rhodes, J., ...
Measurements of X-ray scaling laws are critical for improving cosmological constraints derived with the halo mass function and for understanding the physical processes that govern the heating and...
Galaxy cluster searches by photometric redshifts in the CFHTLS (2009)
Adami, C., Durret, F., Benoist, C., Coupon, J., Mazure, A., Meneux, B., ...
In order to enlarge publicly available optical cluster catalogs, in particular at high redshift, we have performed a systematic search for clusters of galaxies in the CFHTLS. We used the Le Phare...
McCracken, H. J., Capak, P., Salvato, M., Aussel, H., Thompson, D., Daddi, E., ...
(abridged) We present a new near-infrared survey covering the 2 deg sq COSMOS field. Combining our survey with Subaru B and z images we construct a deep, wide-field optical-infrared catalogue. At Ks
Capak, P., Mobasher, B., Scoville, N. Z., McCracken, H., Ilbert, O., Salvato, M., ...
We present three bright z dropout candidates selected from deep Near-Infrared (NIR) imaging of the COSMOS 2 square degree field. All three objects match the 0.8-8um colors of other published z>7...
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...
Floc'h, E. Le, Aussel, H., Ilbert, O., Riguccini, L., Frayer, D., Salvato, M., ...
We present the first results obtained from the identification of ~30,000 sources in the 24mic observations of the COSMOS field at S24>~80muJy. Using accurate photo-z's and extrapolations of the...
Stellar and Total Baryon Mass Fractions in Groups and Clusters Since Redshift 1 (2009)
Giodini, S., Pierini, D., Finoguenov, A., Pratt, G. W., Boehringer, H., Leauthaud, A., ...
We investigate if the discrepancy between estimates of the total baryon mass fraction obtained from observations of the cosmic microwave background (CMB) and of galaxy groups/clusters persists when a...
Jouvel, S., Kneib, J.-P., Ilbert, O., Bernstein, G., Arnouts, S., Dahlen, T., ...
Context. Future dark energy space missions such as JDEM and EUCLID are being designed to survey the galaxy population to trace the geometry of the universe and the growth of structure, which both...
Taniguchi, Y., Murayama, T., Scoville, N. Z., Sasaki, S. S., Nagao, T., Shioya, Y., ...
We present detailed morphological properties of Lyα emitters (LAEs) at z ≈ 5.7 in the COSMOS field based on Hubble Space Telescope Advanced Camera for Surveys (ACS) data. The ACS imaging in the...
Ideue, Y., Nagao, T., Taniguchi, Y., Shioya, Y., Saito, T., Murayama, T., ...
We investigate the relation between the star formation activity in galaxies and environment at z ≃ 1.2 in the Cosmic Evolution Survey field, using the fraction of [O II] emitters and the local...
Ulmer, M. P., Adami, C., Lima Neto, G. B., Durret, F., Covone, G., Ilbert, O., ...
Context. The cosmic time around the z ~ 1 redshift range appears crucial in the cluster and galaxy evolution, since it is probably the epoch of the first mature galaxy clusters. Our knowledge of the...
Ulmer, M. P., Adami, C., Neto, G. B. Lima, Durret, F., Covone, G., Ilbert, O., ...
The cosmic time around the z~1 redshift range appears crucial in the cluster and galaxy evolution, since it is probably the epoch of the first mature galaxy clusters. Our knowledge of the properties...
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
Very deep spectroscopy of the Coma cluster line of sight: exploring new territories (2009)
Adami, C., Brun, V. Le, Biviano, A., Durret, F., Lamareille, F., Pello, R., ...
Environmental effects have an important influence on cluster galaxies, but studies at very faint magnitudes (R>21) are almost exclusively based on imaging. We present here a very deep spectroscopic...
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...
Star Formation and Dust Obscuration at z ≈ 2: Galaxies at the Dawn of Downsizing (2009)
Pannella, M., Carilli, C. L., Daddi, E., McCracken, H. J., Owen, F. N., Renzini, A., ...
We present first results of a study aimed to constrain the star formation rate (SFR) and dust content of galaxies at z ≈ 2. We use a sample of BzK-selected star-forming galaxies, drawn from the...
HST/ACS Morphology of Lyman Alpha Emitters at Redshift 5.7 in the COSMOS Field (2009)
Taniguchi, Y., Murayama, T., Scoville, N. Z., Sasaki, S. S., Nagao, T., Shioya, Y., ...
We present detailed morphological properties of Lyman alpha emitters (LAEs) at z~ 5.7 in the COSMOS field, based on {\it Hubble Space Telescope} Advanced Camera for Surveys (ACS) data. The ACS...
Environmental Effects on the Star Formation Activity in Galaxies at z=1.2 in the COSMOS Field (2009)
Ideue, Y., Nagao, T., Taniguchi, Y., Shioya, Y., Saito, T., Murayama, T., ...
We investigate the relation between the star-formation activity in galaxies and environment at z=1.2 in the COSMOS field, using the fraction of [OII] emitters and the local galaxy density. The...
Star formation and dust obscuration at z~2: galaxies at the dawn of downsizing (2009)
Pannella, M., Carilli, C. L., Daddi, E., Cracken, H. J. Mc, Owen, F. N., Renzini, A., ...
We present first results of a study aimed to constrain the star formation rate and dust content of galaxies at z~2. We use a sample of BzK-selected star-forming galaxies, drawn from the COSMOS...
Stellar and total baryon mass fractions in groups and clusters since redshift 1 (2009)
Giodini, S., Pierini, D., Finoguenov, A., Pratt, G. W., Boehringer, H., Leauthaud, A., ...
We investigate if the discrepancy between estimates of the total baryon mass fraction obtained from observations of the cosmic microwave background (CMB) and of galaxy groups/clusters persists when a...
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...
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...
Spitzer 70 and 160-micron Observations of the COSMOS Field (2009)
Frayer, D. T., Sanders, D. B., Surace, J. A., Aussel, H., Salvato, M., Floc'h, E. Le, ...
We present Spitzer 70 and 160 micron observations of the COSMOS Spitzer survey (S-COSMOS). The data processing techniques are discussed for the publicly released products consisting of images and...
Jouvel, S., Kneib, J-P., Ilbert, O., Bernstein, G., Arnouts, S., Dahlen, T., ...
Future dark energy space missions such as JDEM and EUCLID are being designed to survey the galaxy population to trace the geometry of the universe and the growth of structure, which both depend on...
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...
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),...
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 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., ...
Stellar and Total Baryon Mass Fractions in Groups and Clusters since Redshift 1 (2009)
Giodini, S., Pierini, D., Finoguenov, A., Pratt, G. W., Boehringer, H., Leauthaud, A., ...
Stellar and total baryon mass fractions in groups and clusters since redshift 1 (2009)
Giodini, S., Pierini, D., Finoguenov, A., Pratt, G. W., Böhringer, H., Leauthaud, A., ...
Tasca, L. A. M., Kneib, J.-P., Iovino, A., Le Fèvre, O., Kovac, K., Bolzonella, M., ...
The zCOSMOS 10k-Bright Spectroscopic Sample (2009)
Lilly, S. J., LeBrun, V., Maier, C., Mainieri, V., Mignoli, M., Scodeggio, M., ...
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., ...
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., ...
Spitzer 70 and 160 μm Observations of the COSMOS Field (2009)
Frayer, D. T., Sanders, D. B., Surace, J. A., Aussel, H., Salvato, M., Le Floc'h, E., ...
Jouvel, S., Kneib, J.-P., Ilbert, O., Bernstein, G., Arnouts, S., Dahlen, T., ...
Star Formation and Dust Obscuration at z ≈ 2: Galaxies at the Dawn of Downsizing (2009)
Pannella, M., Carilli, C. L., Daddi, E., McCracken, H. J., Owen, F. N., Renzini, A., ...
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...
Spitzer 70 and 160 μm observations of the COSMOS field (2009)
Frayer, D. T., Sanders, D. B., Surace, J. A., Aussel, H., Salvato, M., Le Floc'h, E., ...
We present Spitzer 70 and 160 mum observations of the COSMOS Spitzer survey (S-COSMOS). The data processing techniques are discussed for the publicly released products consisting of images and source...
Star formation and dust obscuration at z = 2: galaxies at the dawn of downsizing (2009)
Pannella, M., Carilli, C. L., Daddi, E., McCracken, H. J., Owen, F. N., Renzini, A., ...
We present first results of a study aimed to constrain the star formation rate (SFR) and dust content of galaxies at z ââ°Ë 2. We use a sample of BzK-selected star-forming galaxies, drawn...
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...
Taniguchi, Y., Murayama, T., Scoville, N. Z., Sasaki, S. S., Nagao, T., Shioya, Y., ...
We present detailed morphological properties of Lyalpha emitters (LAEs) at z ââ°Ë 5.7 in the COSMOS field based on Hubble Space Telescope Advanced Camera for Surveys (ACS) data. The ACS...
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...
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...
Dust-enshrouded star formation in XMM-LSS galaxy clusters (2008)
Temporin, S., Duc, P. -A., Ilbert, O., Collaboration, The XMM-LSS/SWIRE
We present an investigation of the dust-enshrouded activity in a sample of X-ray selected clusters drawn from the XMM-LSS survey in the redshift range z ~ 0.05 - 1.05. By taking advantage of the...
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...
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...
Orientations of very faint galaxies in the Coma cluster (2008)
Adami, C., Gavazzi, R., Cuillandre, J. C., Durret, F., Ilbert, O., Mazure, A., ...
We have then searched for preferential orientations of faint galaxies in the Coma cluster (down I_Vega~-11.5). By applying a deconvolution method to deep u* and I band images of the Coma cluster, we...
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 redshifts as a tool to study the Coma cluster galaxy populations (2008)
Adami, C., Ilbert, O., Pello, R., Cuillandre, J. C., Durret, F., Mazure, A., ...
We investigate the Coma cluster galaxy luminosity function (GLF) at faint magnitudes, in particular in the u* band by applying photometric redshift techniques applied to deep u*, B, V, R, I images...
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,...
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...
Spectroscopic confirmation of an extreme starburst at redshift 4.547 (2008)
Capak, Peter, Carilli, C. L., Lee, N., Aldcroft, T., Aussel, H., Schinnerer, E., ...
We report the spectroscopic confirmation of a submillimeter galaxy (SMG) at z = 4.547 with an estimated LIR = (0.5–2.0) x 10¹³ L☉. The spectra, mid-IR, and X-ray properties indicate the...
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)...
An optical view of the filament region of Abell 85 (2008)
Boué, G., Durret, F., Adami, C., Mamon, G. A., Ilbert, O., Cayatte, V.
We compare the distribution of optically and Halpha (Ha) selected galaxies in the Southern half of the nearby Abell 85 (A85) cluster with the recently discovered X-ray filament (XRF). We search for...
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...
Spectroscopic Confirmation Of An Extreme Starburst At Redshift 4.547 (2008)
Capak, Peter, Carilli, C. L., Lee, N., Aldcroft, T., Aussel, H., Schinnerer, E., ...
We report the spectroscopic confirmation of a sub-mm galaxy (SMG) at z=4.547 with an estimated L_IR=0.5-2.0x10^13 L_sun. The spectra, mid-IR, and X-ray properties indicate the bolometric luminosity...
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, De La Torre, S., ...
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...
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...
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...
A test of the nature of cosmic acceleration using galaxy redshift distortions (2008)
L. Guzzo, M. Pierleoni, B. Meneux, E. Branchini, O. Le Fèvre, C. Marinoni, ...
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., ...
Garilli, B., Le Fèvre, O., Guzzo, L., Maccagni, D., Le Brun, V., De La Torre, S., ...
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., ...
Clusters at redshift beyond 1.5 in the COSMOS field (2008)
Salvato, M., Guzzo, G., Finoguenov, A., Giodini, S., Scoville, N., Hasinger, G., ...
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)...
Spectroscopic confirmation of an extreme starburst at redshift 4.547 (2008)
Capak, Peter, Carilli, C. L., Lee, N., Aldcroft, T., Aussel, H., Schinnerer, E., ...
We report the spectroscopic confirmation of a submillimeter galaxy (SMG) at z=4.547 with an estimated LIR = (0.5-2.0) Ã 1013 Lsolar. The spectra, mid-IR, and X-ray properties indicate the...
Very weak lensing in the CFHTLS Wide: Cosmology from cosmic shear in the linear regime (2007)
Fu, L., Semboloni, E., Hoekstra, H., Kilbinger, M., Van Waerbeke, L., Tereno, I., ...
We present an exploration of weak lensing by large-scale structure in the linear regime, using the third-year (T0003) CFHTLS Wide data release. Our results place tight constraints on the scaling of...
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
De La Torre, S., Le Fèvre, O., Arnouts, S., Guzzo, L., Farrah, D., Iovino, A., ...
Aims. By combining data from the VIMOS VLT Deep Survey (VVDS) with the Spitzer Wide-area InfraRed Extragalactic survey (SWIRE), we have built the currently largest spectroscopic sample of high...
Zamojski, M. A., Schiminovich, D., Rich , R. M., Mobasher, B., Koekemoer, A. M., Capak, P., ...
We present a study of the morphological nature of redshift z ~ 0.7 star-forming galaxies using a combination of HST ACS, GALEX, and ground-based images of the COSMOS field. Our sample consists of...
Sanders, D. B., Salvato, M., Aussel, H., Ilbert, O., Scoville, N., Surace, J. A., ...
The COSMOS Spitzer survey (S-COSMOS) is a Legacy program (Cycles 2+3) designed to carry out a uniform deep survey of the full 2 deg^2 COSMOS field in all seven Spitzer bands (3.6, 4.5, 5.6, 8.0,...
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...
Mazure, A., Adami, C., Pierre, M., Le Fèvre, O., Arnouts, S., Duc, P. A., ...
We investigate structures in the D1 CFHTLS deep field in order to test the method that will be applied to generate homogeneous samples of clusters and groups of galaxies in order to constrain...
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)...
Mazure, A, Adami, C, Pierre, M, Le Fevre, O, Arnouts, S, Duc, PA, ...
Aims. We investigate structures in the D1 CFHTLS deep field to test the method that will be applied to generate homogeneous samples of clusters and groups of galaxies in order to constrain the...
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,...
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...
Zamojski, M. A., Schiminovich, D., Rich, R. M., Mobasher, B., Koekemoer, A. M., Capak, P., ...
We present a study of the morphological nature of redshift z~0.7 star-forming galaxies using a combination of HST/ACS, GALEX and ground-based images of the COSMOS field. Our sample consists of 8,146...
De La Torre, S., 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...
Sanders, D. B., Salvato, M., Aussel, H., Ilbert, O., Scoville, N., Surace, J. A., ...
The Spitzer-COSMOS survey (S-COSMOS) is a Legacy program (Cycles 2+3) designed to carry out a uniform deep survey of the full 2 sq deg COSMOS field in all seven Spitzer bands (3.6, 4.5, 5.6, 8.0,...
Mazure, A., Adami, C., Pierre, M., Fèvre, O. Le, Arnouts, S., Duc, P. A., ...
We investigate structures in the D1 CFHTLS deep field in order to test the method that will be applied to generate homogeneous samples of clusters and groups of galaxies in order to constrain...
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...
Photometric Redshifts of Galaxies in COSMOS (2007)
Mobasher, B., Capak, P., Scoville, N. Z., Dahlen, T., Salvato, M., Aussel, H., ...
We measure photometric redshifts and spectral types for galaxies in the COSMOS survey. We use template fitting technique combined with luminosity function priors and with the option to simultaneously...
VVDS-SWIRE: Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2 (2007)
De La Torre, S., 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...
Zamojski, M. A., Schiminovich, D., Rich, R. M., Mobasher, B., Koekemoer, A. M., Capak, P., ...
We present a study of the morphological nature of redshift z~0.7 star-forming galaxies using a combination of HST/ACS, GALEX and ground-based images of the COSMOS field. Our sample consists of 8,146...
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
Sanders, D. B., Salvato, M., Aussel, H., Ilbert, O., Scoville, N., Surace, J. A., ...
The Spitzer-COSMOS survey (S-COSMOS) is a Legacy program (Cycles 2+3) designed to carry out a uniform deep survey of the full 2 sq deg COSMOS field in all seven Spitzer bands (3.6, 4.5, 5.6, 8.0,...
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., ...
Photometric redshifts of galaxies in COSMOS (2007)
Mobasher, B., Capak, P., Scoville, N. Z., Dahlen, T., Salvato, M., Aussel, H., ...
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., ...
De La Torre, S., 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., ...
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., ...
Sanders, D. B., Salvato, M., Aussel, H., Ilbert, O., Scoville, N., Surace, J. A., ...
The COSMOS Spitzer survey (S-COSMOS) is a Legacy program (Cycles 2+3) designed to carry out a uniform deep survey of the full 2 deg2 COSMOS field in all seven Spitzer bands (3.6, 4.5, 5.6, 8.0, 24.0,...
Sanders, D. B., Salvato, M., Aussel, H., Ilbert, O., Scoville, N., Surace, J. A., ...
The Spitzer-COSMOS survey (S-COSMOS) is a Legacy program (Cycles 2+3) designed to carry out a uniform deep survey of the full 2 sq deg COSMOS field in all seven Spitzer bands (3.6, 4.5, 5.6, 8.0,...
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...
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., ...
M. A. Zamojski, D. Schiminovich, R. M. Rich, B. Mobasher, A. M. Koekemoer, P. Capak, ...
We present a study of the morphological nature of redshift z ∼ 0.7 star-forming galaxies using a combination of HST/ACS, GALEX and ground-based images of the COSMOS field. Our sample consists of...
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...
Photometric Redshifts of Galaxies in COSMOS (2006)
Mobasher, B., Capak, P., Scoville, N. Z., Dahlen, T., Salvato, M., Aussel, H., ...
We measure photometric redshifts and spectral types for galaxies in the COSMOS survey. We use template fitting technique combined with luminosity function priors and with the option to simultaneously...
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 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
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...
GALEX Detection of Lyman Break Galaxies at z=1 in the CDFS (2006)
Burgarella, D., Perez-Gonzalez, P., Buat, V., Takeuchi, T. T., Lauger, S., Rieke, G., ...
The first large sample of Lyman Break Galaxies (LBGs) at z~1 is selected from GALEX Far-UV and Near-UV images of the Chandra Deep Field South. This multi-wavelength study is based on the wealth of...
Burgarella, D., Perez-Gonzalez, P. G., Tyler, K. D., Rieke, G. H., Buat, V., Takeuchi, T. T., ...
We present the first large, unbiased sample of Lyman Break Galaxies (LBGs) at z ~ 1. Far ultraviolet-dropout (1530 A) galaxies in the Chandra Deep Field South have been selected using GALEX data....
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...
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 Vimos VLT Deep Survey: Compact structures in the CDFS (2006)
Adami, C., Mazure, A., Ilbert, O., Cappi, A.
We have used the Vimos VLT Deep Survey in combination with other spectroscopic, photometric and X-ray surveys from literature to detect several galaxy structures in the Chandra Deep Field South...
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., Brun, D. Bottini V. Le, 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
Burgarella, D., Perez-Gonzalez, P. G., Tyler, K. D., Rieke, G. H., Buat, V., Takeuchi, T. T., ...
We present the first large, unbiased sample of Lyman Break Galaxies (LBGs) at z ~ 1. Far ultraviolet-dropout (1530 A) galaxies in the Chandra Deep Field South have been selected using GALEX data....
Burgarella, D., Perez-Gonzalez, P. G., Tyler, K. D., Rieke, G. H., Buat, V., Takeuchi, T. T., ...
We present the first large, unbiased sample of Lyman Break Galaxies (LBGs) at z ~ 1. Far ultraviolet-dropout (1530 A) galaxies in the Chandra Deep Field South have been selected using GALEX data....
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...
Burgarella, D., Perez-Gonzalez, P. G., Tyler, K. D., Rieke, G. H., Buat, V., Takeuchi, T. T., ...
We present the first large, unbiased sample of Lyman Break Galaxies (LBGs) at z ~ 1. Far ultraviolet-dropout (1530 A) galaxies in the Chandra Deep Field South have been selected using GALEX data....
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...
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., ...
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)
O. Le Fèvre, S. Paltani, S. Arnouts, S. Charlot, S. Foucaud, O. Ilbert, ...
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...
GALEX Detection of Lyman Break Galaxies at z=1 in the CDFS (2005)
Burgarella, D., Perez-Gonzalez, P., Buat, V., Takeuchi, T. T., Lauger, S., Rieke, G., ...
The first large sample of Lyman Break Galaxies (LBGs) at z~1 is selected from GALEX Far-UV and Near-UV images of the Chandra Deep Field South. This multi-wavelength study is based on the wealth of...
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 GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function (2005)
Arnouts, S., Schiminovich, D., Ilbert, O., Tresse, L., Milliard, B., Treyer, M., ...
We present the first measurement of the galaxy luminosity function at 1500A between 0.2
The Vimos VLT Deep Survey: Compact structures in the CDFS (2005)
Adami, C., Mazure, A., Ilbert, O., Cappi, A., Consortium, The VVDS
We have used the Vimos VLT Deep Survey in combination with other spectroscopic, photometric and X-ray surveys from literature to detect several galaxy structures in the Chandra Deep Field South...
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 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,...
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...
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: Compact structures in the CDFS (2005)
Adami, C., Mazure, A., Ilbert, O., Cappi, A.
We have used the Vimos VLT Deep Survey in combination with other spectroscopic, photometric and X-ray surveys from literature to detect several galaxy structures in the Chandra Deep Field South...
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., Brun, D. Bottini V. Le, 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...
Arnouts, S., Schiminovich, D., Ilbert, O., Tresse, L., Milliard, B., Treyer, M., ...
We present the first measurement of the galaxy luminosity function (LF) at 1500 Å in the range 0.2
GALEX Detection of Lyman Break Galaxies at z=1 in the CDFS (2005)
Burgarella, D., Perez-Gonzalez, P., Buat, V., Takeuchi, T. T., Lauger, S., Rieke, G., ...
The first large sample of Lyman Break Galaxies (LBGs) at z~1 is selected from GALEX Far-UV and Near-UV images of the Chandra Deep Field South. This multi-wavelength study is based on the wealth of...
GALEX Detection of Lyman Break Galaxies at z=1 in the CDFS (2005)
Burgarella, D., Perez-Gonzalez, P., Buat, V., Takeuchi, T. T., Lauger, S., Rieke, G., ...
The first large sample of Lyman Break Galaxies (LBGs) at z~1 is selected from GALEX Far-UV and Near-UV images of the Chandra Deep Field South. This multi-wavelength study is based on the wealth of...
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: Compact structures in the CDFS (2005)
Adami, C., Mazure, A., Ilbert, O., Cappi, A.
We have used the Vimos VLT Deep Survey in combination with other spectroscopic, photometric and X-ray surveys from literature to detect several galaxy structures in the Chandra Deep Field South...
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., Brun, D. Bottini V. Le, 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 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 GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function (2004)
Arnouts, S., Schiminovich, D., Ilbert, O., Tresse, L., Milliard, B., Treyer, M., ...
We present the first measurement of the galaxy luminosity function at 1500A between 0.2
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...
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...
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., Brun, D. Bottini V. Le, 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...
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 GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function (2004)
Arnouts, S., Schiminovich, D., Ilbert, O., Tresse, L., Milliard, B., Treyer, M., ...
We present the first measurement of the galaxy luminosity function at 1500A between 0.2
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 GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function (2004)
Arnouts, S., Schiminovich, D., Ilbert, O., Tresse, L., Milliard, B., Treyer, M., ...
We present the first measurement of the galaxy luminosity function at 1500A between 0.2
Deep redshift surveys : The VIMOS VLT deep surveys (2004)
Le Fevre, O., Vettlani,, G., Maccagni, D., Picat, J. P., Adami, C., Arnoboldi, M., ...
Le Fevre, Olivier, Ilbert, O., Marinnoni,, C., Paltani, S., Vettolani, G., Tresse, L., ...
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...