@article{10902/13871,
year = {2014},
url = {http://hdl.handle.net/10902/13871},
abstract = {The "Seyfert and star formation Activity in the Far-Infrared" (SAFIR) project is aimed at studying the physical nature of the nuclear IR emission and star formation properties of a small sample of nearby Seyfert galaxies observed with the PACS and SPIRE instruments on board the Herschel space observatory. In this paper, we review the achieved results, that reveal the importance of the far-IR range to improve the quality and reliability of the estimates of basic AGN torus parameters, and describe some preliminary outcome from the on-going work on the dust properties of resolved AGN host galaxies.},
publisher = {Czech Technical University},
publisher = {Acta Polytechnica CTU Proceedings, Vol.1, Num. 1, Pp. 307-310 (2014)},
title = {Recent Results from the SAFIR Project},
author = {Sánchez-Portal, M. and Castillo Fraile, M. and Ramos Almeida, Cristina and Esquej, P. and Alonso Herrero, Almudena and Pérez García, A.M. and Acosta Pulido, José and Altieri, B. and Bongiovanni, A. and Castro Cerón, J. M. and Cepa, Jordi and Coia, D. and Conversi, L. and Fritz, J. and González Serrano, José Ignacio and Hatziminaoglou, E. and Rodríguez, Espinosa, J. M. and Valtchanov, I.},
}