activity
19992021
most citedPACS Evolutionary Probe (PEP) - A Herschel Key Program

503 citations · 2.6k across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.GA2021★ 48 cited

COALAS: I. ATCA CO(1-0) survey and luminosity function in the Spiderweb protocluster at z=2.16

S. Jin, H. Dannerbauer, B. Emonts +25

We report a detailed CO(1-0) survey of a galaxy protocluster field at , based on 475 hours of observations with the Australia Telescope Compact Array. We constructed a larg…

astro-ph.IM2017★ 25 cited

The Herschel/PACS Point Source Catalogue Explanatory Supplement

G. Marton, L. Calzoletti, A. M. Perez Garcia +6

The Herschel Space Observatory was the fourth cornerstone mission in the European Space Agency (ESA) science programme. It had excellent broad band imaging capabilities in the far-…

astro-ph.CO2013★ 208 cited

The suppression of star formation by powerful active galactic nuclei

M. J. Page, M. Symeonidis, J. D. Vieira +75

The old, red stars which constitute the bulges of galaxies, and the massive black holes at their centres, are the relics of a period in cosmic history when galaxies formed stars at…

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★ 34 cited

The lack of star formation gradients in galaxy groups up to z~1.6

Felicia Ziparo, Paola Popesso, Andrea Biviano +28

In the local Universe, galaxy properties show a strong dependence on environment. In cluster cores, early type galaxies dominate, whereas star-forming galaxies are more and more co…

astro-ph.CO2011★ 66 cited

The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel

P. Popesso, A. Biviano, G. Rodighiero +40

Star formation in massive galaxies is quenched at some point during hierarchical mass assembly. To understand where and when the quenching processes takes place, we study the evolu…