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Table 6.

Classification of the host galaxies of the GTC and VLT samples based on their dynamical state and morphology.

Short galaxy ID Dynamical Morphological class Reference
class (visual or parametric)
(1) (2) (3) (4)
OSIRIS/GTC

0741+3020 Intermediate (U)LIRG–E/S0 Multiple system This work
0818+3958 E/S0 Uncertain This work
0834+5534 E/S0 E This work
0902+5459a E/S0 Uncertain This work
0956+5735 E/S0 E UM19
1101+4004a E/S0 Double system This work

FORS2/VLT

J0923+0101 E/S0 E UM19
J0950+0111 E/S0 Possibly 2 nuclei VM16, This work
J0955+0346 E/S0 E This work
J1014+0244 E/S0 Uncertain This work
J1153+0326 E/S0 E? This work
J1247+0152 E/S0 E This work
J1307–0214 E/S0 Highly disturbed This work
J1336–0039 E/S0 E This work
J1337–0128 E/S0 Highly disturbed UM19
J1407+0217 E/S0 E UM19
J1413–0142 E/S0 E G09
J1430–0050 Uncertain Highly disturbed VM12
J1546–0005 E/S0 E UM19

Notes. Dynamical and morphological classifications of the AGN host galaxies in the GTC and VLT samples. Column (1): short SDSS galaxy ID. Column (2): dynamical classification according to the values derived in Tables 4 and 3 in B13. Column (3): morphological classification according to the visual inspection of SDSS and/or HST images (this work) or parametrical analyses (G09, VM12, VM16, UM19: Greene et al. 2009; Villar-Martín et al. 2012, 2016; Urbano-Mayorgas et al. 2019, respectively). The results based on the parametric classification are differentiated from the visual classification results with italic font. Column (4): reference for the morphological classification in Col. (3). Both classification methods show that none of the galaxies are classified as spirals or disks, neither dynamically nor morphologically.

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