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19962012
most citedStar Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies

2k citations · 9.3k across the 65 of their papers we have counts for

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Showing 2004 · astro-phShow all

11 papers · 2 filters

astro-ph2004

Optical and near-infrared properties of submillimetre galaxies in the GOODS-North field

Alexandra Pope, Douglas Scott, Colin Borys +3

We investigate the photometric redshift distribution, colours and morphologies of a large sample of submillimetre sources in the GOODS-North region. With the depth achieved by the…

astro-ph2004

The Structural Properties of Isolated Galaxies, Spiral-Spiral Pairs, and Mergers: The Robustness of Galaxy Morphology During Secular Evolution

H. Hernandez-Toledo, V. Avila-Reese, C. J. Conselice +1

We present a structural analysis of nearby galaxies in spiral-spiral pairs in optical BVRI bands and compare with the structures of isolated spiral galaxies and galaxies in ongoing…

astro-ph2004

X-ray Properties of Lyman Break Galaxies in the Great Observatories Origins Deep Survey

B. D. Lehmer, W. N. Brandt, D. M. Alexander +9

We constrain the X-ray emission properties of Lyman break galaxies (LBGs) at z ~ 3-6 using the 2 Ms Chandra Deep Field-North and 1 Ms Chandra Deep Field-South. Large samples of LBG…

astro-ph2004

Large scale diffuse light in the Coma cluster: a multi-scale approach

C. Adami, E. Slezak, F. Durret +7

We have obtained wide field images of the Coma cluster in the B, V, R and I bands with the CFH12K camera at CFHT. In order to search for large scale diffuse emission, we have appli…

astro-ph2004

Obscured AGN and the X-ray, Optical and Far-Infrared Number Counts of AGN in the GOODS Fields

E. Treister, C. M. Urry, E. Chatzichristou +12

The deep X-ray, optical, and far-infrared fields that constitute GOODS are sensitive to obscured AGN (N_H>10^{22} cm^{-2}) at the quasar epoch (z~2-3), as well as to unobscured AGN…

astro-ph2004

Bar Evolution Over the Last Eight Billion Years: A Constant Fraction of Strong Bars in GEMS

S. Jogee, F. D. Barazza, H. -W. Rix +25

One third of present-day spirals host optically visible strong bars that drive their dynamical evolution. However, the fundamental question of how bars evolve over cosmological tim…