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An overview of the lightning and atmospheric electricity observations collected in southern France during the HYdrological cycle in Mediterranean EXperiment (HyMeX), Special Observation Period 1

The PEACH project (Projet en Electricité Atmosphérique pour la Campagne HyMeX – the Atmospheric Electricity Project of the HyMeX Program) is the atmospheric electricity component of the Hydrology cycle in the Mediterranean Experiment (HyMeX) experiment and is dedicated to the observation of both lightning activity and electrical state of continental and maritime thunderstorms in...

Structure detection in the D1 CFHTLS deep field using accurate photometric redshifts: a benchmark

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 cosmology and detailed physics of groups and clusters.Methods.An adaptive kernel technique was applied to galaxy catalogues. This technique needs none of the usual a-priori assumptions...

Structure detection in the D1 CFHTLS deep field using accurate photometric redshifts: a benchmark

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 cosmology and detailed physics of groups and clusters.Methods.An adaptive kernel technique was applied to galaxy catalogues. This technique needs none of the usual a-priori assumptions...

Bias in the estimation of global luminosity functions

We discuss a bias present in the calculation of the global luminosity function (LF) which occurs when analysing faint galaxy samples. This effect exists as a result of the different spectral energy distributions of galaxies, which are in turn quantified by the k corrections. We demonstrate that this bias occurs because not all galaxy types are visible in the same absolute...

Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering

A&A Astronomy & Astrophysics S. de la Torre B. Meneux G. De Lucia J. Blaizot O. Le Fèvre B. Garilli O. Cucciati Y. Mellier A. Pollo U. Abbas D. Bottini V. Le Brun D. Maccagni M. Scodeggio L. Tresse

The VIMOS-VLT deep survey: the group catalogue

A&A Astronomy & Astrophysics O. Cucciati C. Marinoni A. Iovino S. Bardelli C. Adami A. Mazure M. Scodeggio D. Maccagni S. Temporin E. Zucca G. De Lucia J. Blaizot B. Garilli B. Meneux G. Zamorani O

The VVDS-SWIRE-GALEX-CFHTLS surveys: physical properties of galaxies at z below 1.2 from photometric data

. Iovino H. J. McCracken B. Marano C. Marinoni A. Mazure B. Meneux R. Merighi S. Paltani R. Pellò A. Pollo M. Radovich E. Zucca C. Lonsdale C. Martin Measuring the build-up of stellar mass is one of the

The VIMOS-VLT Deep Survey: evolution in the halo occupation number since z∼ 1*

U. Abbas 16 18 S. de la Torre 15 18 22 O. Le F e`vre 18 L. Guzzo 15 20 21 C. Marinoni 19 B. Meneux 21 24 A. Pollo 17 23 G. Zamorani 7 D. Bottini 22 B. Garilli 22 V. Le Brun 18 D. Maccagni 22 R

The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z≃ 1

. Meneux 17 18 U. Abbas 16 L. Tasca 11 C. M. Carollo 21 T. Contini 20 J.-P. Kneib 14 S. J. Lilly 21 V. Mainieri 15 A. Renzini 8 M. Scodeggio 11 G. Zamorani 9 S. Bardelli 9 M. Bolzonella 9 A. Bongiorno 18 K

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

. J. McCracken B. Marano C. Marinoni A. Mazure B. Meneux R. Merighi S. Paltani R. Pellò A. Pollo L. Pozzetti M. Radovich D. Vergani G. Zamorani E. Zucca M. Bondi A. Bongiorno J. Brinchmann O. Cucciati S

The VIMOS-VLT Deep Survey (VVDS) - The dependence of clustering on galaxy stellar mass at z ~ 1

A&A The VIMOS-VLT Deep Survey (VVDS) B. Meneux L. Guzzo B. Garilli O. Le Fèvre A. Pollo J. Blaizot G. De Lucia M. Bolzonella F. Lamareille L. Pozzetti A. Cappi A. Iovino C. Marinoni H. J. McCracken

The VIMOS VLT Deep Survey - Tracing the galaxy stellar mass assembly history over the last 8 Gyr

Aims. Our aim is to investigate the history of mass assembly for galaxies of different stellar masses and types.Methods. We selected a mass-limited sample of 4048 objects from the VIMOS VLT Deep Survey (VVDS) in the redshift interval . We then used an empirical criterion, based on the amplitude of the 4000 ÅBalmer break (Dn4000), to separate the galaxy population into...

The VIMOS VLT Deep Survey - The assembly history of the stellar mass in galaxies: from the young to the old universe

B. Marano C. Marinoni A. Mazure B. Meneux R. Merighi S. Paltani R. Pellò A. Pollo M. Radovich M. Bondi A. Bongiorno O. Cucciati S. de la Torre L. Gregorini Y. Mellier P. Merluzzi D. Vergani C. J

The zCOSMOS survey. The dependence of clustering on luminosity and stellar mass at –1

A&A Astronomy & Astrophysics B. Meneux L. Guzzo S. de la Torre C. Porciani G. Zamorani U. Abbas M. Bolzonella B. Garilli A. Iovino L. Pozzetti E. Zucca S. J. Lilly O. Le Fèvre J.-P. Kneib C. M

The VIMOS VLT deep survey - The ultraviolet galaxy luminosity function and luminosity density at 3 4

Aims.We study the luminosity function of the high-redshift galaxy population with redshifts  using a purely I-band magnitude-selected spectroscopic sample obtained in the framework of the VIMOS VLT Deep Survey (VVDS).Methods.We determine the luminosity function from the VVDS, taking care to add as few assumptions and as simple corrections as possible, and compare our results with...

The VIMOS VLT deep survey - First epoch VVDS-deep survey: 11 564 spectra with 17.5 ≤ I ≤ 24, and the redshift distribution over 0 ≤ z ≤ 5

. Marano C. Marinoni G. Mathez A. Mazure B. Meneux R. Merighi S. Paltani R. Pellò A. Pollo L. Pozzetti M. Radovich G. Zamorani E. Zucca M. Bondi A. Bongiorno G. Busarello F. Lamareille Y. Mellier P. Merluzzi

The VIMOS-VLT deep survey - Evolution of the galaxy luminosity function up to z = 2 in first epoch data

. Marano C. Marinoni G. Mathez A. Mazure B. Meneux R. Merighi S. Paltani R. Pello A. Pollo M. Radovich M. Bondi A. Bongiorno G. Busarello P. Ciliegi F. Lamareille Y. Mellier P. Merluzzi V. Ripepi D. Rizzo

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

11 O. Cucciati 10 S. Foucaud 4 P. Franzetti 15 I. Gavignaud 5 L. Guzzo 15 B. Marano 8 C. Marinoni 2 7 A. Mazure 7 B. Meneux 15 R. Merighi 12 S. Paltani 0 3 A. Pollo 7 L. Pozzetti 12 M. Radovich 1 E

The VIMOS VLT Deep Survey - Evolution of the luminosity functions by galaxy type up to z = 1.5 from first epoch data

I. Gavignaud L. Guzzo A. Iovino B. Marano C. Marinoni A. Mazure B. Meneux R. Merighi S. Paltani R. Pellò A. Pollo M. Radovich M. Bondi A. Bongiorno G. Busarello O. Cucciati L. Gregorini F. Lamareille

The VIMOS-VLT Deep Survey - Galaxy luminosity function per morphological type up to z = 1.2

Aims.We have computed the evolution of the rest-frame B-band luminosity function (LF) for bulge and disk-dominated galaxies since .Methods.We use a sample of 605 spectroscopic redshifts with in the Chandra Deep Field South from the VIMOS-VLT Deep Survey, 3555 galaxies with photometric redshifts from the COMBO-17 multi-color data, coupled with multi-color HST/ACS images from the...