activity
20062021
most citedThe lesser role of starbursts for star formation at z=2

867 citations · 14.6k across the 138 of their papers we have counts for

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Showing 2011Show all

20 papers · 1 filter

astro-ph.CO2011★ 10 cited

Spitzer IRAC identification of Herschel-ATLAS SPIRE sources

Sam Kim, Julie L. Wardlow, Asantha Cooray +28

We use spitzer-IRAC data to identify near-infrared counterparts to submillimeter galaxies detected with Herschel-SPIRE at 250um in the Herschel Astrophysical Terahertz Large Area S…

astro-ph.CO2011★ 66 cited

The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel

P. Popesso, A. Biviano, G. Rodighiero +40

Star formation in massive galaxies is quenched at some point during hierarchical mass assembly. To understand where and when the quenching processes takes place, we study the evolu…

astro-ph.CO2011★ 119 cited

H-ATLAS/GAMA: Dusty early-type galaxies and passive spirals

K. Rowlands, L. Dunne, S. Maddox +38

We present the dust properties and star-formation histories of local submillimetre-selected galaxies in Herschel-ATLAS, classified by optical morphology. The early-type galaxies (E…

astro-ph.CO2011★ 54 cited

The red-sequence of 72 WINGS local galaxy clusters

T. Valentinuzzi, B. M. Poggianti, G. Fasano +14

We study the color-magnitude red sequence and blue fraction of 72 X-ray selected galaxy clusters at z=0.04-0.07 from the WINGS survey, searching for correlations between the charac…

astro-ph.CO2011★ 80 cited

Morphology of galaxies in the WINGS clusters

G. Fasano, E. Vanzella, A. Dressler +12

We present the morphological catalog of galaxies in nearby clusters of the WINGS survey (Fasano et al. 2006). The catalog contains a total number of 39923 galaxies, for which we pr…

astro-ph.CO2011★ 113 cited

The Herschel Multi-Tiered Extragalactic Survey: SPIRE-mm Photometric Redshifts

I. G. Roseboom, R. J. Ivison, T. R. Greve +78

We investigate the potential of submm-mm and submm-mm-radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500 μm by the SPIRE instrument on He…