Table 1
Sample of IR bright Seyfert galaxies observed with Herschel/SPIRE FTS.
Galaxy name | RA | Dec | cza | DLb | Nuclear | log LIRd | αAGNe | Obs. IDf | |||
(J2000.0) | (J2000.0) | (km s-1) | (Mpc) | spect. class.c | (L⊙) | (%) | |||||
|
|||||||||||
NGC 34 | 00 11 06.5 | −12 06 26 | 5881 | 77.0 | Sy2 | 11.4 | 2 | 1342199253 | |||
IRASF 05189–2524 | 05 21 01.4 | −25 21 45 | 12760 | 181 | Sy2 | 12.2 | 71 | 1342192832, 1342192833 | |||
UGC 05101 | 09 35 51.6 | +61 21 11 | 11802 | 168 | Sy2 | 12.0 | 35 | 1342209278 | |||
NGC 5135 | 13 25 44.0 | −29 50 01 | 4105 | 60.9 | Sy2 | 11.3 | 20 | 1342212344 | |||
NGC 7130 | 21 48 19.5 | −34 57 04 | 4842 | 63.6 | Sy2 | 11.3 | 25 | 1342219565 | |||
NGC 7469 | 23 03 15.6 | +08 52 26 | 4892 | 56.6 | Sy1 | 11.5 | 20 | 1342199252 |
Notes.
Classification of the nuclear activity from optical spectroscopy from Yuan et al. (2010), except for NGC 7469 (Alonso-Herrero et al. 2009).
Logarithm of the IR luminosity, L(8–1000 μm), from Sanders et al. (2003) scaled to the adopted distance.
AGN fractional contribution to the total luminosity from Esquej et al. (2012), Veilleux et al. (2009), and Pereira-Santaella et al. (2011).
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