Enhanced star formation rates in AGN hosts with respect to inactive galaxies 
from PEP-Herschel observations

Santini, P.; Rosario, D. J.; Shao, L.; Lutz, D.; Maiolino, R.; Alexander, D. M.; Altieri, B.; Andreani, P.; Aussel, H.; Bauer, F. E.; Berta, S.; Bongiovanni, A.; Brandt, W. N.; Brusa, M.; Cepa, J.; Cimatti, A.; Daddi, E.; Elbaz, D.; Fontana, A.; Förster Schreiber, N. M.; Genzel, R.; Grazian, A.; Le Floc'h, E.; Magnelli, B.; Mainieri, V.; Nordon, R.; Perez Garcia, A. M.; Poglitsch, A.; Popesso, P.; Pozzi, F.; Riguccini, L.; Rodighiero, G.; Salvato, M.; Sanchez-Portal, M.; Sturm, E.; Tacconi, L. J.; Valtchanov, I.; Wuyts, S.

doi:10.1051/0004-6361/201118266

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Enhanced star formation rates in AGN hosts with respect to inactive galaxies from PEP-Herschel observations

Santini, P., Rosario, D. J., Shao, L., Lutz, D., Maiolino, R., Alexander, D. M., et al. (2012). Enhanced star formation rates in AGN hosts with respect to inactive galaxies from PEP-Herschel observations. Astronomy & Astrophysics, 540: A109 (20pp). doi:10.1051/0004-6361/201118266.

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Urheber:
Santini, P.¹, Autor
Rosario, D. J.¹, Autor
Shao, L.², Autor
Lutz, D.¹, Autor
Maiolino, R.¹, Autor
Alexander, D. M.¹, Autor
Altieri, B.¹, Autor
Andreani, P.¹, Autor
Aussel, H.¹, Autor
Bauer, F. E.¹, Autor
Berta, S.¹, Autor
Bongiovanni, A.¹, Autor
Brandt, W. N.¹, Autor
Brusa, M.¹, Autor
Cepa, J.¹, Autor
Cimatti, A.¹, Autor
Daddi, E.¹, Autor
Elbaz, D.¹, Autor
Fontana, A.¹, Autor
Förster Schreiber, N. M.¹, Autor
Genzel, R.¹, AutorGrazian, A.¹, AutorLe Floc'h, E.¹, AutorMagnelli, B.¹, AutorMainieri, V.¹, AutorNordon, R.¹, AutorPerez Garcia, A. M.¹, AutorPoglitsch, A.¹, AutorPopesso, P.¹, AutorPozzi, F.¹, AutorRiguccini, L.¹, AutorRodighiero, G.¹, AutorSalvato, M.^{3, 4}, Autor Sanchez-Portal, M.¹, AutorSturm, E.¹, AutorTacconi, L. J.¹, AutorValtchanov, I.¹, AutorWuyts, S.¹, Autor mehr..

Affiliations:
1Max-Planck-Institut für Extraterrestrische Physik (MPE), Postfach 1312, 85741 Garching, Germany; INAF – Osservatorio Astronomico di Roma, via di Frascati 33, 00040 Monte Porzio Catone, Italy; Department of Physics, Durham University, South Road, Durham, DH1 3LE, UK; European Space Astronomy Centre, Villafranca del Castillo, Spain; ESO, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany; INAF – Osservatorio Astronomico di Trieste, via Tiepolo 11, 34131 Trieste, Italy; Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, IRFU/Service d’Astrophysique, Bât. 709, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France; Pontificia Universidad Católica de Chile, Departamento de Astronomía y Astrofísica, Casilla 306, Santiago 22, Chile; Instituto de Astrofísica de Canarias, 38205 La Laguna, Spain; Departamento de Astrofísica, Universidad de La Laguna, Spain; Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, University Park, PA 16802, USA; Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, 40127 Bologna, Italy; Dipartimento di Astronomia, Università di Padova, Vicolo dell’Osservatorio 3, 35122 Padova, Italy, ou_persistent22
2Plasma Edge and Wall (E2M), Max Planck Institute for Plasma Physics, Max Planck Society, ou_1856327
3Group 'Astrophysics and Laboratory Plasma Studies' (ALPS), Max Planck Institute for Plasma Physics, Max Planck Society, ou_1856335
4Office of the Director (DI), Max Planck Institute for Plasma Physics, Max Planck Society, ou_1856325