output
19932026
most citedThe Sloan Digital Sky Survey: Technical Summary

10.4k citations

Showing 2005Show all

72 papers · 1 filter

astro-ph2005★ 10 cited

Deviations from passive evolution - star formation and the UV excess in z~1 radio galaxies

K. J. Inskip, P. N. Best, M. S. Longair

Galaxy colours are determined for two samples of 6C and 3CR radio sources at z~1, differing by a factor of ~6 in radio power. Corrections are made for emission line contamination a…

astro-ph2005★ 308 cited

The evolution of the star formation activity in galaxies and its dependence on environment

B. M. Poggianti, A. von der Linden, G. De Lucia +16

We study how the proportion of star-forming galaxies evolves between z=0.8 and z=0 as a function of galaxy environment, using the [OII] line in emission as a signature of ongoing s…

astro-ph2005★ 7 cited

Imaging and integral field spectroscopy of shocked H2 around G25.65+1.05

S. P. Todd, S. K. Ramsay Howat

Near-infrared imaging of the emission from molecular hydrogen is a powerful method for discovering outflows in star-forming regions. We present new near-infrared images, long slit…

astro-ph2005★ 84 cited

An Overdensity of Galaxies near the Most Distant Radio-Loud Quasar

W. Zheng, R. Overzier, R. J. Bouwens +41

A five square arcminute region around the luminous radio-loud quasar SDSS J0836+0054 (z=5.8) hosts a wealth of associated galaxies, characterized by very red (1.3 < i_775 - z_{850}…

astro-ph2005★ 83 cited

Further constraints on the evolution of Ks-selected galaxies in the GOODS/CDFS field

K. I. Caputi, R. J. McLure, J. S. Dunlop +2

We have selected and analysed the properties of a sample of 2905 Ks<21.5 galaxies in ~ 131 sq.arcmin of the Great Observatories Origins Deep Survey (GOODS) Chandra Deep Field South…

astro-ph2005★ 532 cited

High-resolution Millimeter Imaging of Submillimeter Galaxies

L. J. Tacconi, R. Neri, S. C. Chapman +8

We present sub-arcsecond resolution IRAM PdBI interferometry of eight submillimeter galaxies at redshifts from 2 to 3.4, where we detect continuum at 1mm and/or CO lines at 3 and 1…