Ulisse: A tool for one-shot sky exploration and its application for detection of active galactic nuclei

Abstract

Context.Modern sky surveys are producing ever larger amounts of observational data, which makes the application of classical approaches for the classification and analysis of objects challenging and time consuming. However, this issue may be significantly mitigated by the application of automatic machine and deep learning methods.Aims.We proposeulisse, a new deep learning tool that, starting from a single prototype object, is capable of identifying objects that share common morphological and photometric properties, and hence of creating a list of candidate lookalikes. In this work, we focus on applying our method to the detection of active galactic nuclei (AGN) candidates in a Sloan Digital Sky Survey galaxy sample, because the identification and classification of AGN in the optical band still remains a challenging task in extragalactic astronomy.Methods.Intended for the initial exploration of large sky surveys,ulissedirectly uses features extracted from the ImageNet dataset to perform a similarity search. The method is capable of rapidly identifying a list of candidates, starting from only a single image of a given prototype, without the need for any time-consuming neural network training.Results.Our experiments showulisseis able to identify AGN candidates based on a combination of host galaxy morphology, color, and the presence of a central nuclear source, with a retrieval efficiency ranging from 21% to 65% (including composite sources) depending on the prototype, where the random guess baseline is 12%. We findulisseto be most effective in retrieving AGN in early-type host galaxies, as opposed to prototypes with spiral- or late-type properties.Conclusions.Based on the results described in this work,ulissecould be a promising tool for selecting different types of astro-physical objects in current and future wide-field surveys (e.g.,Euclid, LSST etc.) that target millions of sources every single night.