867 citations · 9.9k across the 173 of their papers we have counts for
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CO luminosity function from Herschel-selected galaxies and the contribution of AGN
L. Vallini, C. Gruppioni, F. Pozzi +2
We derive the CO luminosity function (LF) for different rotational transitions (i.e. (1-0), (3-2), (5-4)) starting from the Herschel LF by Gruppioni et al. and using appropriate $L…
The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV & [OII]λ3727 luminosities
M. Talia, A. Cimatti, L. Pozzetti +7
We use a spectroscopic sample of 286 star-forming galaxies (SFGs) at 1<z<3 from the GMASS survey to study different star formation rate (SFR) estimators. Infrared (IR) data are use…
Dust attenuation in z 1 galaxies from Herschel and 3D-HST H measurements
A. Puglisi, G. Rodighiero, A. Franceschini +12
We combined the spectroscopic information from the 3D-HST survey with \textit{Herschel} data to characterize the H dust attenuation properties of a sample of 79 main sequence st…
Predictions for surveys with the SPICA Mid-infrared Instrument
M. Bonato, M. Negrello, Z. -Y. Cai +8
We present predictions for number counts and redshift distributions of galaxies detectable in continuum and in emission lines with the Mid-infrared (MIR) Instrument (SMI) proposed…
Star Formation in Herschel's Monsters versus Semi-Analytic Models
C. Gruppioni, F. Calura, F. Pozzi +9
We present a direct comparison between the observed star formation rate functions (SFRF) and the state-of-the-art predictions of semi-analytic models (SAM) of galaxy formation and…
The most obscured AGN in the COSMOS field
G. Lanzuisi, M. Perna, I. Delvecchio +11
Highly obscured active galactic nuclei (AGN) are common in nearby galaxies, but are difficult to observe beyond the local Universe, where they are expected to significantly contrib…