activity
19992021
most citedThe Infrared Astronomical Mission AKARI

842 citations · 1.2k across the 13 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2021★ 18 cited

Late-time radio observations of the short GRB200522A: constraints on the magnetar model

G. Bruni, B. O'Connor, T. Matsumoto +4

GRB200522A is a short duration gamma-ray burst (GRB) at redshift =0.554 characterized by a bright infrared counterpart. A possible, although not unambiguous, interpretation of t…

astro-ph.EP2021★ 19 cited

Measurements of the Zodiacal Light Absolute Intensity through Fraunhofer Absorption Line Spectroscopy with CIBER

Phillip Korngut, Min Gyu Kim, Toshiaki Arai +14

Scattered sunlight from the interplanetary dust (IPD) cloud in our Solar system presents a serious foreground challenge for spectro-photometric measurements of the Extragalactic Ba…

astro-ph.EP2018★ 26 cited

Zodiacal Light Beyond Earth Orbit Observed with Pioneer 10

T. Matsumoto, K. Tsumura, Y. Matsuoka +1

We reanalyze the Imaging Photopolarimeter data from Pioneer 10 to study the zodiacal light in the B and R bands beyond Earth orbit, applying an improved method to subtract integrat…

astro-ph.GA2018★ 16 cited

MIRIS observation of near-infrared diffuse Galactic light

Y. Onishi, K. Sano, S. Matsuura +17

We report near-infrared (IR) observations of high Galactic latitude clouds to investigate diffuse Galactic light (DGL), which is starlight scattered by interstellar dust grains. Th…

astro-ph.GA2017★ 27 cited

Spitzer Observations of the North Ecliptic Pole

H. Nayyeri, N. Ghotbi, A. Cooray +19

We present a photometric catalog for Spitzer Space Telescope warm mission observations of the North Ecliptic Pole (NEP; centered at , $\rm Decl.=66^d33^m38^s…

astro-ph.CO2015★ 28 cited

AKARI Observation of the Sub-degree Scale Fluctuation of the Near-infrared Background

H. J. Seo, Hyung Mok Lee, T. Matsumoto +3

We report spatial fluctuation analysis of the sky brightness in near-infrared from observations toward the north ecliptic pole (NEP) by the AKARI at 2.4 and 3.2 micron. As a follow…