activity
20112022
most citedOptical - Near-Infrared catalogue for the AKARI North Ecliptic Pole Deep Field

43 citations · 138 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.IM2022★ 3 cited

Deblurring galaxy images with Tikhonov regularization on magnitude domain

Kazumi Murata, Tsutomu T. Takeuchi

We propose a regularization-based deblurring method that works efficiently for galaxy images. The spatial resolution of a ground-based telescope is generally limited by seeing cond…

astro-ph.IM2021★ 14 cited

Hyper Suprime-Cam Legacy Archive

Masayuki Tanaka, Hiroyuki Ikeda, Kazumi Murata +5

We present the launch of the Hyper Suprime-Cam Legacy Archive (HSCLA), a public archive of processed, science-ready data from Hyper Suprime-Cam (HSC). HSC is an optical wide-field…

astro-ph.IM2019★ 5 cited

AGN selection in the AKARI NEP deep field with the fuzzy SVM algorithm

Artem Poliszczuk, Aleksandra Solarz, Agnieszka Pollo +14

The aim of this work is to create a new catalog of reliable AGN candidates selected from the AKARI NEP-Deep field. Selection of the AGN candidates was done by applying a fuzzy SVM…

astro-ph.GA2017

North Ecliptic Pole multi-wavelength survey : new optical data with Hyper Suprime-Cam and near-future prospects with eROSITA

Nagisa Oi, Hideo Matsuhara, Tomotsugu Goto +19

The AKARI North Ecliptic Pole (NEP) survey consists of two survey projects: NEP-Deep (0.5 sq.deg) and NEP-Wide (5.4 sq.deg), providing with tens of thousands of galaxies. A continu…

astro-ph.GA2017

Overview of North Ecliptic Pole Deep multi-wavelength Survey (NEP-Deep)

H. Matsuhara, T. Wada, N. Oi +22

The recent updates of the North Ecliptic Pole deep (0.5~deg, NEP-Deep) multi-wavelength survey covering from X-ray to radio-wave is presented. The NEP-Deep provides us with sev…

astro-ph.GA2017★ 1 cited

NEP-AKARI: Evolution with redshift of dust attenuation in 8 micron selected galaxies

V. Buat, N. Oi, D. Burgarella +8

We built a 8um selected sample of galaxies in the NEP-AKARI field by defining 4 redshift bins with the four AKARI bands at 11, 15, 18 and 24 microns (0.15<z<0.49, 0.75<z<1.34, 1.34…