activity
19982026
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 49.3k across the 379 of their papers we have counts for

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Showing 2005Show all

14 papers · 1 filter

astro-ph2005★ 15 cited

An investigation of the submillimeter background radiation using SCUBA and Spitzer

S. Dye, S. A. Eales, M. L. N. Ashby +8

We investigate the redshift dependence of the contribution to the extragalactic far-infrared/sub-millimeter background from galaxies detected by the Spitzer Space Telescope at 8um…

astro-ph2005★ 63 cited

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★ 87 cited

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★ 30 cited

Stellar populations in the CFHTLS. I. New constraints on the IMF at low mass

M. Schultheis, A. C. Robin, C. Reylé +4

We present a stellar populations analysis of the first release of the CFHTLS (Canada-France-Hawai Telescope Legacy Survey) data. A detailed comparison between the Besançon model of…

astro-ph2005★ 51 cited

A large population of galaxies 9 to 12 billion years back in the history of the Universe

O. Le Fevre, S. Paltani, S. Arnouts +6

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 Univers…

astro-ph2005★ 53 cited

An H-band survey of the Herschel Deep Field

N. Metcalfe, T. Shanks, P. M. Weilbacher +3

We present H-band infra-red galaxy data to a 3 sigma limit of H=22.9 and optical-infra-red colours of galaxies on the William Herschel Deep Field. These data were taken from a 7'x…