activity
20102023
most citedThe Mean Star Formation Rate of X-ray selected Active Galaxies and its Evolution from z=2.5: Results from PEP-Herschel

299 citations · 308 across the 2 of their papers we have counts for

collaborators

13 papers

hep-ex2023★ 9 cited

Terrestrial Very-Long-Baseline Atom Interferometry: Workshop Summary

Sven Abend, Baptiste Allard, Iván Alonso +250

This document presents a summary of the 2023 Terrestrial Very-Long-Baseline Atom Interferometry Workshop hosted by CERN. The workshop brought together experts from around the world…

astro-ph.CO2012★ 299 cited

The Mean Star Formation Rate of X-ray selected Active Galaxies and its Evolution from z=2.5: Results from PEP-Herschel

D. J. Rosario, P. Santini, D. Lutz +37

(Abridged) We study relationships between the SFR and the nuclear properties of X-ray selected AGNs out to z=2.5, using far-IR data in three extragalactic deep fields as part of th…

astro-ph.CO2012

Enhanced star formation rates in AGN hosts with respect to inactive galaxies from PEP-Herschel observations

P. Santini, D. J. Rosario, L. Shao +35

We compare the average star formation (SF) activity in X-ray selected AGN hosts with mass-matched control inactive galaxies,including star forming and quiescent sources, at 0.5<z<2…

astro-ph.CO2011

PACS Evolutionary Probe (PEP) - A Herschel Key Program

D. Lutz, A. Poglitsch, B. Altieri +35

Deep far-infrared photometric surveys studying galaxy evolution and the nature of the cosmic infrared background are a key strength of the Herschel mission. We describe the scienti…

astro-ph.CO2010

Evolution of Dust Temperature of Galaxies through Cosmic Time as seen by Herschel

H. S. Hwang, D. Elbaz, G. E. Magdis +112

We study the dust properties of galaxies in the redshift range 0.1<z<2.8 observed by the Herschel Space Observatory in the field of the Great Observatories Origins Deep Survey-Nort…

astro-ph.CO2010

Herschel FIR counterparts of selected Ly-alpha emitters at z~2.2. Fast evolution since z~3 or missed obscured AGNs?

A. Bongiovanni, I. Oteo, J. Cepa +58

Ly-alpha emitters (LAEs) are seen everywhere in the redshift domain from local to z~7. Far-infrared (FIR) counterparts of LAEs at different epochs could provide direct clues on dus…