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Table 4:

Classification from optical lines in the nuclear ( $r \leq r _e$/16) region.

Galaxy Id
Emission typea Activity Classb
NGC 128 H LINER
NGC 777 W Sy/ LINER
NGC 1052 H LINER
NGC 1209 H LINER
NGC 1297 H LINER
NGC 1366 N  
NGC 1380 H LINER
NGC 1389 N  
NGC 1407 N  
NGC 1426 N  
NGC 1453 H LINER
NGC 1521 W LINER
NGC 1533 H LINER
NGC 1553 W LINER
NGC 1947 H LINER
NGC 2749 H LINER
NGC 2911 H LINER
NGC 2962 H  
NGC 2974 H LINER
NGC 3136 H LINER/ Sy
NGC 3258 H Comp
NGC 3268 H LINER
NGC 3489 H Sy/ LINER
NGC 3557 W LINER
NGC 3607 H LINER
NGC 3818 Traces  
NGC 3962 H LINER
NGC 4374 H LINER
NGC 4552 W Comp
NGC 4636 H LINER
NGC 4696 H LINER
NGC 4697 W LINER
NGC 5011 W LINER
NGC 5044 H LINER
NGC 5077 H LINER
NGC 5090 H LINER
NGC 5193 W Comp
NGC 5266 H LINER
NGC 5328 W/Traces Comp
NGC 5363 H LINER
NGC 5638 N  
NGC 5812 N  
NGC 5813 W LINER
NGC 5831 N  
NGC 5846 H LINER
NGC 5898 W LINER
NGC 6721 W/Traces Comp
NGC 6758 H LINER
NGC 6776 H LINER/ Sy
NGC 6868 H LINER
NGC 6875 W  
NGC 6876 W /Traces Comp
NGC 6958 H Sy/ LINER
NGC 7007 W Sy/ LINER
NGC 7079 W LINER
NGC 7097 H LINER
NGC 7135 H LINER
NGC 7192 W LINER
NGC 7332 W/Traces  
NGC 7377 W LINER
IC 1459 H LINER
IC 2006 W Comp
IC 3370 H LINER
IC 4296 H LINER
IC 5063 H Sy

Notes. (a) N = no emission; W = weak emission ( $EW({\rm H}\alpha + {\rm [NII]}6584)<3$ Å); H = high emission ( $ EW({\rm H}\alpha + {\rm [NII]6584)>} 3$ Å). (b) At larger radii, some LINERs are classified as composites.


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