Finding binary active galactic nuclei candidates by the centroid shift in imaging surveys II. Testing the method with SDSS J233635.75-010733.7

TL;DR

This study verifies a centroid shift method for identifying binary active galactic nuclei (AGNs) using imaging survey data, demonstrating its effectiveness with SDSS J233635.75-010733.7 and proposing a new comparative approach across different bands.

Contribution

The paper tests and confirms the centroid shift technique for binary AGN detection and introduces a new band comparison method for systems with different spectral energy distributions.

Findings

Detected positional dispersion excess in PTF data for the known binary AGN.

Significant position differences between g and R bands indicate the method's effectiveness.

Method is promising for large-scale surveys to find binary AGN candidates.

Abstract

In Liu (2015), we propose selecting binary active galactic nuclei (AGNs) candidates using the centroid shift of the images, which 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 ability of this method. Using 162 exposures in the $R$ band of \textit{Palomar Transient Factory} (PTF), an excess of dispersion in the positional distribution of the binary AGN is detected, though 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 the difference is highly significant even only with 20 exposures. This new method is efficient for two nuclei with different spectral energy distributions, e.g., type I + type II AGN or off-set AGN. Large-scale surveys, e.g., 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.