Authors: Ivano Baronchelli, G. Rodighiero, Harry I. Teplitz, Claudia Scarlata, Alberto Franceschini, S. Berta, Laia Barrufet, Mattia Vaccari, Matteo Bonato, Laure Ciesla, A. Zanella, R. Carraro, Chiara Mancini, A. Puglisi, M. A. Malkan, Simona Mei, Lucia Marchetti, James W. Colbert, Chris Sedgwick, Steve Serjeant, Chris Pearson, M. Radovich, A. Grado, L. Limatola, Giovanni Covone
Venue: The Astrophysical Journal
Type: Publication
Abstract: For a sample of star forming galaxies in the redshift interval 0.15$<$z$<$0.3, we study how both the relative strength of the AGN infra-red emission, compared to that due to the star formation (SF), and the numerical fraction of AGNs, change as a function of the total stellar mass of the hosting galaxy group (M$^{*}_{\mathrm{group}}$), between $10^{10.25}$ and $10^{11.9}$M$_{\odot}$. Using a multi-component SED fitting analysis, we separate the contribution of stars, AGN torus and star formation to the total emission at different wavelengths. T...
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Topics: 
Astrophysics
Astronomy
DOI:
10.3847/1538-4357/aab78b
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