Where's Swimmy?: Mining unique color features buried in galaxies by deep anomaly detection using Subaru Hyper Suprime-Cam data
Takumi S. Tanaka, Rhythm Shimakawa, Kazuhiro Shimasaku, Yoshiki Toba,, Nobunari Kashikawa, Masayuki Tanaka, Akio K. Inoue

TL;DR
This paper introduces Swimmy, a deep-learning anomaly detection method applied to Subaru Hyper Suprime-Cam data, effectively identifying rare and unique galaxy populations without labeled training data, and revealing their physical and morphological properties.
Contribution
The paper presents a novel deep anomaly detection technique tailored for wide-field galaxy imaging data, successfully identifying rare objects like XELGs and quasars without prior labels.
Findings
Successfully detected 60-70% of quasars and 60% of XELGs as anomalies
Identified galaxies with unique morphological features
Demonstrated deep anomaly detection as an effective tool for discovering rare astronomical objects
Abstract
We present the Swimmy (Subaru WIde-field Machine-learning anoMalY) survey program, a deep-learning-based search for unique sources using multicolored () imaging data from the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP). This program aims to detect unexpected, novel, and rare populations and phenomena, by utilizing the deep imaging data acquired from the wide-field coverage of the HSC-SSP. This article, as the first paper in the Swimmy series, describes an anomaly detection technique to select unique populations as "outliers" from the data-set. The model was tested with known extreme emission-line galaxies (XELGs) and quasars, which consequently confirmed that the proposed method successfully selected 60-70% of the quasars and 60% of the XELGs without labeled training data. In reference to the spectral information of local galaxies at 0.05-0.2 obtained from the Sloan…
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