Table 1
Physical properties and observed frequency ranges for our six target AGN.
| Object | Typea | Redshift | M• [108 M⊙] | kpc-morphology | α | ν [GHz] | ν0 [GHz] | |
|
|
||||||||
| 0415+379 (3C 111) | Sy 1 | 0.049 | 36b | 2-sided jet | 0.9 ± 0.1 | 84–227 | 88–238 | |
| 0507+179 | QSO | 0.416 | 2c | 1-sided jet | 0.3 ± 0.1 | 84–231 | 120–326 | |
| 0528+134 (OG+134) | HPQ | 2.060 | 10d | 2-sided jet | 0.9 ± 0.1 | 84–231 | 258–705 | |
| 0954+658 | BL Lac | 0.367 | 3e | 1-sided jet | 0.3 ± 0.1 | 82–235 | 112–321 | |
| 1418+546 (OQ+530) | BL Lac | 0.153 | 9f | 1-sided halo | 0.2 ± 0.1 | 82–253 | 95–291 | |
| 1637+574 (OS+562) | Sy 1 | 0.751 | 17g | 1-sided halo | 0.1 ± 0.3 | 80–115 | 141–201 | |
Notes. Source types, redshifts, and kpc-morphology are taken from the NED and the MOJAVE database (Lister et al. 2009). Black hole masses M• are taken from the corresponding references. We give the ranges of observed frequencies ν as well as the corresponding rest-frame frequencies ν0. Millimeter spectral indices α are taken from Paper I; they are defined via Sν ∝ ν − α.
Marchesini et al. (2004).
D’Elia et al. (2003).
Ghisellini et al. (2009).
Fan & Cao (2004).
Falomo et al. (2003).
Liu et al. (2006).
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