Panchromatic spectral energy distributions of simulated galaxies: results at redshift z=0
David Goz, Pierluigi Monaco, Gian Luigi Granato, Giuseppe Murante, Rosa Dominguez-Tenreiro, Aura Obreja, Marianna Annunziatella, Edoardo Tescari
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | OXFORD UNIV PRESS | Published : 2017
We present predictions of spectral energy distributions (SEDs), from the UV to the FIR, of simulated galaxies at z = 0. These were obtained by post-processing the results of an N-body+hydro simulation of a cosmological box of side 25 Mpc, which uses the Multi-Phase Particle Integrator (MUPPI) for star formation and stellar feedback, with the GRASIL-3D radiative transfer code that includes reprocessing of UV light by dust. Physical properties of our sample of ∼500 galaxies resemble observed ones, though with some tension at small and large stellar masses. Comparing predicted SEDs of simulated galaxies with different samples of local galaxies, we find that these resemble observed ones, when no..View full abstract
Awarded by MINECO (Spain) from PNAyA
Awarded by Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO)
This work is supported by the PRIN-INAF 2012 grant 'The Universe in a Box: Multi-scale Simulations of Cosmic Structures'. The simulations were carried out at the 'Centro Interuniversitario del Nord-Est per il Calcolo Elettronico' (CINECA, Bologna), with CPU time assigned under University-of-Trieste/CINECA and ISCRA grants; the analysis was performed on the facility PICO at CINECA under the ISCRA grant IscrC_GALPP.We thank the MICINN and MINECO (Spain) for grants AYA2009-12792-C03-03 and AYA2012-31101 from the PNAyA. AO was financially supported through a FPI contract from MINECO (Spain).Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020. This work was supported by the Flagship Allocation Scheme of the NCI National Facility at the ANU.