918 citations · 20.3k across the 303 of their papers we have counts for
14 papers · 1 filter
Simulating the infrared sky with a Spritz
L. Bisigello, C. Gruppioni, A. Feltre +6
Current hydrodynamical and semi-empirical simulations of galaxy formation and evolution have difficulties in reproducing the number densities of IR-detected galaxies. Therefore, a…
The infrared-radio correlation of star-forming galaxies is strongly M-dependent but nearly redshift-invariant since z4
I. Delvecchio, E. Daddi, M. T. Sargent +25
Several works in the past decade have used the ratio between total (rest 8-1000m) infrared and radio (rest 1.4~GHz) luminosity in star-forming galaxies (q), often referre…
Co-evolution of black hole accretion and star formation in galaxies up to z=3.5
R. Carraro, G. Rodighiero, P. Cassata +15
We study the co-evolution between the black hole accretion rate (BHAR) and the star formation rate (SFR) in different galaxy life phases: main sequence star-forming galaxies, quies…
Identification of single spectral lines through supervised machine learning in a large HST survey (WISP): a pilot study for Euclid and WFIRST
I. Baronchelli, C. M. Scarlata, G. Rodighiero +13
Future surveys focusing on understanding the nature of dark energy (e.g., Euclid and WFIRST) will cover large fractions of the extragalactic sky in near-IR slitless spectroscopy. T…
The dust and cold gas content of local star forming galaxies
P. Popesso, A. Concas, L. Morselli +3
We use dust masses () derived from far-infrared data and molecular gas masses () based on CO luminosity, to calibrate proxies based on a combination of the galax…
The ALPINE-ALMA [CII] Survey: The nature, luminosity function and star formation history of dusty galaxies up to z~6
C. Gruppioni, M. Bethermin, F. Loiacono +30
We present the detailed characterisation of a sample of 56 sources serendipitously detected in ALMA band 7, as part of the ALMA Large Program to INvestigate CII at Early Times (ALP…