activity
20102014
most citedThe Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4

440 citations · 1.2k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2014★ 189 cited

The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M* plane up to z 2

B. Magnelli, R. J. Ivison, D. Lutz +21

[Abridged] We study the evolution of the radio spectral index and far-infrared/radio correlation (FRC) across the star-formation rate-stellar masse (i.e. SFR-M*) plane up to z 2. W…

astro-ph.CO2013★ 440 cited

The Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4

C. Gruppioni, F. Pozzi, G. Rodighiero +100

We exploit the deep and extended far infrared data sets (at 70, 100 and 160 um) of the Herschel GTO PACS Evolutionary Probe (PEP) Survey, in combination with the HERschel Multi tie…

astro-ph.CO2012★ 33 cited

The AGN content in luminous IR galaxies at z\sim2 from a global SED analysis including Herschel data

F. Pozzi, C. Vignali, C. Gruppioni +16

We use Herschel-PACS far-infrared data, combined with previous multi-band information and mid-IR spectra, to properly account for the presence of an active nucleus and constrain it…

astro-ph.CO2010★ 201 cited

Herschel unveils a puzzling uniformity of distant dusty galaxies

D. Elbaz, H. S. Hwang, B. Magnelli +106

The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their…

astro-ph.CO2010★ 80 cited

PEP: first Herschel probe of dusty galaxy evolution up to z~3

C. Gruppioni, F. Pozzi, P. Andreani +32

We exploit the deepest existing far-infrared (FIR) data obtained so far by Herschel at 100 and 160 um in the GOODS-N, as part of the PACS Evolutionary Probe (PEP) survey, to derive…

astro-ph.CO2010★ 249 cited

The far-infrared/radio correlation as probed by Herschel

R. J. Ivison, B. Magnelli, E. Ibar +100

We set out to determine the ratio, q(IR), of rest-frame 8-1000um flux, S(IR), to monochromatic radio flux, S(1.4GHz), for galaxies selected at far-IR and radio wavelengths, to sear…