NGC 1713: the radial velocity profile of this galaxy reveals a definite KDC in
the centre of this galaxy.
Bright X-ray source (Bauer et al. 2000) and low FIR/radio ratio based
on the Knapp et al. (1989) FIR upper limits indicate that the radio
source is powered by an AGN.
Paired with 04 56.2 -00 33 = NGC 1709 at 2.7, 284, 0.9 x 0.7, compact, m=15.6