activity
20022026
most citedThe lesser role of starbursts for star formation at z=2

867 citations · 17.3k across the 189 of their papers we have counts for

collaborators
Showing 2013Show all

22 papers · 1 filter

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★ 43 cited

Reversal or no reversal: the evolution of the star formation rate-density relation up to z~1.6

F. Ziparo, P. Popesso, A. Finoguenov +27

We investigate the evolution of the star formation rate (SFR)-density relation in the Extended Chandra Deep Field South (ECDFS) and the Great Observatories Origin Deep Survey (GOOD…

astro-ph.CO2013★ 130 cited

The Mean Star-Forming Properties of QSO Host Galaxies

D. J. Rosario, B. Trakhtenbrot, D. Lutz +22

Quasi-stellar objects (QSOs) occur in galaxies in which supermassive black holes (SMBHs) are growing substantially through rapid accretion of gas. Many popular models of the co-evo…