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19982024
most citedCOSMOS Photometric Redshifts with 30-bands for 2-deg2

1.2k citations · 5.6k across the 82 of their papers we have counts for

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Showing 2005Show all

8 papers · 1 filter

astro-ph2005

The VIMOS-VLT Deep Survey: Luminosity dependence of clustering at z~1

A. Pollo, L. Guzzo, O. Le Fevre +2

We investigate the dependence of galaxy clustering on the galaxy intrinsic luminosity at high redshift, using the data from the First Epoch VIMOS-VLT Deep Survey (VVDS). The size (…

astro-ph2005

The VIMOS-VLT Deep Survey - The evolution of galaxy clustering per spectral type to z~1.5

B. Meneux, O. LeFevre, L. Guzzo +47

We measure the evolution of clustering for galaxies with different spectral types from 6495 galaxies with 17.5<=I_AB<=24 and measured spectroscopic redshift in the first epoch VIMO…

astro-ph2005

The Arecibo Legacy Fast ALFA Survey: I. Science Goals, Survey Design and Strategy

Riccardo Giovanelli, Martha P. Haynes, Brian R. Kent

The recently initiated Arecibo Legacy Fast ALFA (ALFALFA) survey aims to map 7000 square degrees of the high galactic latitude sky visible from Arecibo, providing a HI line spectra…

astro-ph2005

The Vimos VLT Deep Survey: Compact structures in the CDFS

C. Adami, A. Mazure, O. Ilbert +2

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 Dee…

astro-ph2005

The VIRMOS deep imaging survey IV: Near-infrared observations

A. Iovino, H. J. McCracken, B. Garilli +49

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 spectr…

astro-ph2005

The VVDS-VLA Deep Field II. Optical and near infrared identifications of VLA S(1.4GHz)>80 microJy sources in the VIMOS VLT Deep Survey VVDS-02h field

P. Ciliegi, G. Zamorani, M. Bondi +46

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 micr…