activity
19982012
most citedzCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field

1k citations · 4.8k across the 35 of their papers we have counts for

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Showing 2008Show all

12 papers · 1 filter

astro-ph200858 cited

AzTEC Millimetre Survey of the COSMOS Field - II. Source Count Overdensity and Correlations with Large-Scale Structure

J. E. Austermann, I. Aretxaga, D. H. Hughes +9

We report an over-density of bright sub-millimetre galaxies (SMGs) in the 0.15 sq. deg. AzTEC/COSMOS survey and a spatial correlation between the SMGs and the optical-IR galaxy den…

astro-ph2008107 cited

The spatial clustering of X-ray selected AGN in the XMM-COSMOS field

R. Gilli, G. Zamorani, T. Miyaji +70

We study the spatial clustering of 538 X-ray selected AGN in the 2 deg^2 XMM-COSMOS field that are spectroscopically identified to I_{AB}<23 and span the redshift range z=0.2-3.0.…

astro-ph200822 cited

Detection of Dense Molecular Gas in Inter-Arm Spurs in M51

S. A. Corder, K. Sheth, N. Z. Scoville +3

Spiral arm spurs are prominent features that have been observed in extinction and 8m emission in nearby galaxies. In order to understand their molecular gas properties, we used…

astro-ph200842 cited

Relation Between Stellar Mass and Star Formation Activity in Galaxies

Bahram Mobasher, T. Dahlen, A. Hopkins +8

For a mass-selected sample of 66544 galaxies with photometric redshifts from the Cosmic Evolution Survey (COSMOS), we examine the evolution of star formation activity as a function…

astro-ph200869 cited

Star formation rates in Lyman break galaxies: radio stacking of LBGs in the COSMOS field and the sub-Jy radio source population

C. L. Carilli, Nicholas Lee, P. Capak +10

We present an analysis of the radio properties of large samples of Lyman Break Galaxies (LBGs) at , 4, and 5 from the COSMOS field. The median stacking analysis yields a…

astro-ph200884 cited

The dust un-biased cosmic star formation history from the 20 cm VLA-COSMOS survey

V. Smolcic, E. Schinnerer, G. Zamorani +8

We derive the cosmic star formation history (CSFH) out to z=1.3 using a sample of ~350 radio-selected star-forming galaxies, a far larger sample than in previous, similar studies.…