We use deep Herschel observations of the complete 2Jy sample of powerful radio active galactic nuclei (AGNs) in the local Universe (0.05 < z 30), consistent with being fuelled by a different mechanism (e.g. the direct accretion of hot gas).
Cone search capability for table J/MNRAS/512/86/2jytab1 (*Properties and dust masses derived with 100/160 microns flux ratios method of the 2Jy sample)
Cone search capability for table J/MNRAS/512/86/3crtab1 (*Properties and dust masses derived with 100/160 microns flux ratios method of the 3CR sample)
Cone search capability for table J/MNRAS/512/86/atlatab1 (*Properties and dust masses derived with 100/160 microns flux ratios method of the Atlas3D sample)
Cone search capability for table J/MNRAS/512/86/hrstab1 (*Properties and dust masses derived with 100/160 microns flux ratios method of the HRS sample)
Cone search capability for table J/MNRAS/512/86/pgqtab1 (*Properties and dust masses derived with 100/160 microns flux ratios method of the PG QSO sample)
Cone search capability for table J/MNRAS/512/86/t2qstab1 (*Properties and dust masses derived with 100/160 microns flux ratios method of Type-II QSO sample)
Cone search capability for table J/MNRAS/512/86/ulirtab1 (*Properties and dust masses derived with 100/160 microns flux ratios method of the ULIRG sample)