We report the discovery of a pair of Seyfert galaxies identified in the ROS
AT bright source, 1RXS J000306.3-041932. The two Seyferts have the same red
shift of 0.106. The angular distance between them is similar to 23 ", corre
sponding to a projected separation of similar to 73 kpc, and suggesting an
interacting system. We argue, from its weak IR emission and relatively larg
e nuclear separation, that the system is an example of the interaction betw
een AGNs, rather than interaction-triggered AGN activity.