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most citedGOODS-Herschel: an infrared main sequence for star-forming galaxies

1.1k citations · 25.3k across the 213 of their papers we have counts for

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106 papers · 1 filter

astro-ph.CO2015★ 26 cited

Passive galaxies as tracers of cluster environments at z~2

V. Strazzullo, E. Daddi, R. Gobat +18

Even 10 billion years ago, the cores of the first galaxy clusters are often found to host a characteristic population of massive galaxies with already suppressed star formation. He…

astro-ph.CO2013★ 285 cited

The evolution of the dust and gas content in galaxies

P. Santini, R. Maiolino, B. Magnelli +36

We use deep Herschel PACS and SPIRE observations in GOODSS, GOODSN and COSMOS to estimate the average dust mass (Mdust) of galaxies on a redshift-stellar mass (Mstar)-SFR grid. We…

astro-ph.CO2013★ 264 cited

The evolution of the dust temperatures of galaxies in the SFR plane up to

B. Magnelli, D. Lutz, A. Saintonge +38

[Abridged] We study the evolution of the dust temperatures of galaxies in the SFR-M* plane up to z~2 using observations from the Herschel Space Observatory. Starting from a sample…

astro-ph.CO2013★ 327 cited

The incidence of obscuration in active galactic nuclei

A. Merloni, A. Bongiorno, M. Brusa +22

We study the incidence of nuclear obscuration on a complete sample of 1310 AGN selected on the basis of their rest-frame 2-10 keV X-ray flux from the XMM-COSMOS survey, in the reds…

astro-ph.CO2013★ 46 cited

Spatially-resolved dust properties of the GRB 980425 host galaxy

Michał J. Michałowski, L. K. Hunt, E. Palazzi +30

Gamma-ray bursts (GRBs) have been proposed as a tool for studying star formation in the Universe, so it is crucial to investigate whether their host galaxies and immediate environm…

astro-ph.CO2013★ 41 cited

Hidden Starbursts and Active Galactic Nuclei at 0<z<4 from the Herschel-VVDS-CFHTLS-D1 Field: Inferences on Coevolution and Feedback

Brian C. Lemaux, Emeric Le Floc'h, Olivier Le Fèvre +12

We investigate of the properties of 2000 Herschel/SPIRE-selected galaxies from using a combination of extensive spectroscopy, deep imaging from CFHT, VLA, Spitzer, XM…