1.1k citations · 4.2k across the 21 of their papers we have counts for
19 papers · 1 filter
Sunyaev-Zel'dovich detection of the galaxy cluster Cl J1449+0856 at z = 1.99: the pressure profile in uv space
R. Gobat, E. Daddi, R. T. Coogan +9
We present Atacama Large Millimetre Array and Atacama Compact Array observations of the Sunyaev-Zel'dovich effect in the z = 2 galaxy cluster Cl J1449+0856, an X-ray-detected proge…
The deepest Herschel-PACS far-infrared survey: number counts and infrared luminosity functions from combined PEP/GOODS-H observations
B. Magnelli, P. Popesso, S. Berta +34
We present results from the deepest Herschel-PACS (Photodetector Array Camera and Spectrometer) far-infrared blank field extragalactic survey, obtained by combining observations of…
Regularity underlying complexity: a redshift-independent description of the continuous variation of galaxy-scale molecular gas properties in the mass-star formation rate plane
Mark T. Sargent, E. Daddi, M. Béthermin +6
Star-forming galaxies (SFGs) display a continuous distribution of specific star formation rates (sSFR) which can be approximated by the superposition of two log-normal distribution…
Panchromatic spectral energy distributions of Herschel sources
S. Berta, D. Lutz, P. Santini +24
(abridged) Far-infrared Herschel photometry from the PEP and HerMES programs is combined with ancillary datasets in the GOODS-N, GOODS-S, and COSMOS fields. Based on this rich data…
The Evolving Interstellar Medium of Star Forming Galaxies Since z=2 as Probed by Their Infrared Spectral Energy Distributions
Georgios E. Magdis, E. Daddi, M. Bethermin +11
Using data from the mid-infrared to millimeter wavelengths for individual galaxies and for stacked ensembles at 0.5<z<2, we derive robust estimates of dust masses (Mdust) for main…
GOODS-Herschel: Ultra-deep XMM-Newton observations reveal AGN/star-formation connection
E. Rovilos, A. Comastri, R. Gilli +30
Models of galaxy evolution assume some connection between the AGN and star formation activity in galaxies. We use the multi-wavelength information of the CDFS to assess this issue.…