摘要：We have previously proposed selecting binary active galactic nuclei (AGNs) candidates
using the centroid shift of the images that is induced by the non-synchronous variations
of the two nuclei. In this paper, a known binary AGN (SDSS J233635.75-010733.7) is
employed to verify the functioning of this method. Using 162 exposures in the
R band of
the Palomar Transient Factory (PTF), an excess of dispersion in the positional
distribution of the binary AGN is detected, although the two nuclei cannot be resolved in
the images of PTF. We also propose a new method to compare the position of the binary AGN
in PTF g and
R band and
find that the difference is highly significant even with only 20 exposures. This new
method is efficient for two nuclei with different spectral energy distributions such as
type I + type II AGN or an off-set AGN. Large-scale surveys such as the Panoramic Survey
Telescope and Rapid Response System, and the Large Synoptic Survey Telescope are expected
to discover a large sample of binary AGN candidates with these methods.
关键词：galaxies: active;astrometry;methods: data analysis
