activity
19942023
most citedThe Cosmic Evolution Survey (COSMOS) -- Overview

2k citations · 32.5k across the 221 of their papers we have counts for

collaborators
Showing 2005Show all

8 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★ 72 cited

Oxygen Gas Abundances at z~1.4: Implications for the Chemical Evolution History of Galaxies

C. Maier, S. J. Lilly, C. M. Carollo +3

The 1<z<2 redshift window hosts the peak of the star formation and metal production rates. Studies of the metal content of the star forming galaxies at these epochs are however spa…

astro-ph2005

GOODS, UDF, and the evolution of early-type galaxies

I. Ferreras, T. Lisker, A. Pasquali +3

The HST/ACS images of GOODS-South have been used to select a sample of early-type galaxies, based on morphology and on the Kormendy relation. The classification scheme does not use…

astro-ph2005

Oxygen Gas Abundances at 0.4<z<1.5: Implications for the Chemical Evolution History of Galaxies

C. Maier, S. J. Lilly, C. M. Carollo

We report VLT-ISAAC and Keck-NIRSPEC near-infrared spectroscopy for a sample of 30 0.47<z<0.92 CFRS galaxies and five [OII]-selected, M_B,AB<-21.5, z~1.4 galaxies. We have measured…

astro-ph2005★ 70 cited

Near-Infrared Spectroscopy of 0.4<z<1.0 CFRS Galaxies: Oxygen Abundances, SFRs and Dust

C. Maier, S. J. Lilly, M. Carollo +2

Using new J-band VLT-ISAAC and Keck-NIRSPEC spectroscopy, we have measured Halpha and [NII] line fluxes for 0.47<z<0.92 CFRS galaxies which have [OII], Hbeta and [OIII]a line fluxe…

astro-ph2005★ 25 cited

XMM-Newton Surveys of the Canada-France Redshift Survey Fields - III: The Environments of X-ray Selected AGN at 0.4<z<0.6

T. J. Waskett, S. A. Eales, W. K. Gear +3

The environmental properties of a sample of 31 hard X-ray selected AGN are investigated, from scales of 500 kpc down to 30 kpc, and are compared to a control sample of inactive gal…