Identification of AKARI infrared sources by Deep HSC Optical Survey: Construction of New Band-Merged Catalogue in the NEP-Wide field
Seong Jin Kim, Nagisa Oi, Tomotsugu Goto, Hiroyuki Ikeda, Simon C.-C., Ho, Hyunjin Shim, Yoshiki Toba, Ho Seong Hwang, Tetsuya Hashimoto, Laia, Barrufet, Matthew Malkan, Helen K. Kim, Ting-Chi Huang, Hideo Matsuhara,, Takamitsu Miyaji, Chris Pearson, Stephen Serjeant

TL;DR
This paper presents a new band-merged catalogue of AKARI infrared sources in the NEP-Wide field, combining multi-wavelength data and identifying faint galaxies through deep optical HSC survey observations.
Contribution
It introduces a comprehensive multi-band photometric catalogue for AKARI sources in the NEP-Wide field, including newly matched faint galaxies with HSC data.
Findings
Identification of 91,861 AKARI sources with multi-band photometry.
Approximately 20,000 new AKARI sources matched to HSC data.
Catalogue covers from UV to submillimetre wavelengths.
Abstract
The north ecliptic pole (NEP) field is a natural deep field location for many satellite observations. It has been targeted manytimes since it was surveyed by the AKARI space telescope with its unique wavelength coverage from the near- to mid-infrared(mid-IR). Many follow-up observations have been carried out and made this field one of the most frequently observed areas witha variety of facilities, accumulating abundant panchromatic data from X-ray to radio wavelength range. Recently, a deep opticalsurvey with the Hyper Suprime-Cam (HSC) at the Subaru telescope covered the NEP-Wide (NEPW) field, which enabled us toidentify faint sources in the near- and mid-IR bands, and to improve the photometric redshift (photo-z) estimation. In this work,we present newly identified AKARI sources by the HSC survey, along with multi-band photometry for 91,861 AKARI sourcesobserved over the NEPW field.…
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