Herschel-SPIRE spectroscopy of nearby Seyfert galaxies

N. Sacchi; H. Roussel; V. Buat; C. D. Wilson; R. Auld; M. J. Barlow; D. Elbaz; W. K. Gear; F. Galliano; L. Cortese; L. Spinoglio; M. Baes; P. Panuzzo; Naseem Rangwala; K. G. Isaak; J. Kamenetzky; T. J. Parkin; S. Charlot; Ανδρέας Παπαγεωργίου; E. Dwek; A. Rykala; L. Ciesla; D. L. Clements; A. Cooray; G. J. Bendo; E. E. Rigby; S. C. Madden; D. Cormier; Ko Okumura; N. Castro-Rodríguez; L. R. Levenson; J. I. Davies; S. A. Eales; J. Glenn; M. J. Page; M. Galametz; S. Oliver; I. Pérez-Fournón; A. Boselli; M. R. P. Schirm; M. Pohlen; B. O’Halloran; M. Bradford; P. Chanial; P. R. Maloney; Matthew Griffin; J. J. Bock; S. Hony; H. L. Gomez; N Lu

Herschel-SPIRE spectroscopy of nearby Seyfert galaxies

N. Sacchi(Roma Tre University), H. Roussel(Centre National de la Recherche Scientifique), V. Buat(Centre National de la Recherche Scientifique), C. D. Wilson(McMaster University), R. Auld(Cardiff University), M. J. Barlow(University College London), D. Elbaz(Université Paris-Saclay), W. K. Gear(Royal Observatory), F. Galliano(Commissariat à l'Énergie Atomique et aux Énergies Alternatives), L. Cortese(The University of Western Australia), L. Spinoglio(National Institute for Astrophysics), M. Baes(HOGENT University of Applied Sciences and Arts), P. Panuzzo(Centre National de la Recherche Scientifique), Naseem Rangwala(University of Colorado Boulder), K. G. Isaak(European Space Research and Technology Centre), J. Kamenetzky(University of Colorado Boulder), T. J. Parkin(McMaster University), S. Charlot(Centre National de la Recherche Scientifique), Ανδρέας Παπαγεωργίου(Cyprus Institute), E. Dwek(Goddard Space Flight Center), A. Rykala(Cardiff University), L. Ciesla(Centre National de la Recherche Scientifique), D. L. Clements(Imperial College London), A. Cooray(University of California, Irvine), G. J. Bendo(University of Manchester), E. E. Rigby(University of Nottingham), S. C. Madden(Centre National de la Recherche Scientifique), D. Cormier(Commissariat à l'Énergie Atomique et aux Énergies Alternatives), Ko Okumura(Juntendo University), N. Castro-Rodríguez(Instituto de Astrofísica de Canarias), L. R. Levenson(California Institute of Technology), J. I. Davies(Cardiff University), S. A. Eales(Cardiff University), J. Glenn(University of Colorado Boulder), M. J. Page(University College London), M. Galametz(Commissariat à l'Énergie Atomique et aux Énergies Alternatives), S. Oliver(University of Sussex), I. Pérez-Fournón(Instituto de Astrofísica de Canarias), A. Boselli(Centre National de la Recherche Scientifique), M. R. P. Schirm(McMaster University), M. Pohlen(Cardiff University), B. O’Halloran(Imperial College London), M. Bradford(California Institute of Technology), P. Chanial, P. R. Maloney, Matthew Griffin(RMIT University), J. J. Bock(Jet Propulsion Laboratory), S. Hony(Institut de Recherche sur les Lois Fondamentales de l'Univers), H. L. Gomez(Cardiff University), N Lu

ORCA Online Research @Cardiff (Cardiff University)

January 15, 2011

Cited by 0

Related Papers

Planck2015 results

|Astronomy and Astrophysics|2016|10.7k

Gaia Data Release 2

|Astronomy and Astrophysics|2018|8.7k

Planck2013 results. XVI. Cosmological parameters

|Astronomy and Astrophysics|2014|6.6k

Planck 2015 results

|Research Explorer (The University of Manchester)|2016|5.5k

Gaia Data Release 3

|Astronomy and Astrophysics|2022|4k