activity
20162026
most citedAn attempt to detect transient changes in Io's SO2 and NaCl atmosphere

29 citations · 61 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM2026

VLBI-Enabled Localization of Continuous GW Sources

Keitaro Takahashi, Takuya Akahori, Kenta Fujisawa +8

Pulsar timing arrays (PTAs) are opening the nanohertz gravitational-wave (GW) band by timing millisecond pulsars (MSPs) to target signals from supermassive black hole binaries (SMB…

astro-ph.EP2023

A search for auroral radio emission from βPictoris b

Yuta Shiohira, Yuka Fujii, Hajime Kita +3

Magnetized exoplanets can serve as the source of auroral radio emissions, allowing us to characterize the magnetospheric properties of these planets. Successful detections of auror…

astro-ph.EP2023★ 1 cited

Revealing the dynamics of magnetosphere, atmosphere, and interior of solar system objects with the Square Kilometre Array

Tomoki Kimura, Yuka Fujii, Hajime Kita +3

Bodies such as planets, moons, and asteroids in our solar system are the brightest objects in the low-frequency radio astronomy at 10 GHz. The low-frequency radio emissi…

astro-ph.EP2021★ 10 cited

Jupiter's X-ray aurora during UV dawn storms and injections as observed by XMM-Newton, Hubble, and Hisaki

A. D. Wibisono, G. Branduardi-Raymont, W. R. Dunn +9

We present results from a multiwavelength observation of Jupiter's northern aurorae, carried out simultaneously by XMM-Newton, the Hubble Space Telescope (HST), and the Hisaki sate…

astro-ph.EP2020★ 29 cited

An attempt to detect transient changes in Io's SO2 and NaCl atmosphere

L. Roth, J. Boissier, A. Moullet +15

Io's atmosphere is predominately SO2 sustained by a combination of volcanic outgassing and sublimation. The loss from the atmosphere is the main mass source for Jupiter's large mag…

astro-ph.HE2016★ 16 cited

Wide-Band Spectra of Giant Radio Pulses from the Crab Pulsar

Ryo Mikami, Katsuaki Asano, Shuta J. Tanaka +9

We present the results of the simultaneous observation of the giant radio pulses (GRPs) from the Crab pulsar at 0.3, 1.6, 2.2, 6.7, and 8.4 GHz with four telescopes in Japan. We ob…

astro-ph.IM2016★ 5 cited

Very Long Baseline Interferometry Experiment on Giant Radio Pulses of Crab Pulsar toward Fast Radio Burst Detection

K. Takefuji, T. Terasawa, T. Kondo +6

We report on a very long baseline interferometry (VLBI) experiment on giant radio pulses (GPs) from the Crab pulsar in the radio 1.4 to 1.7 GHz range to demonstrate a VLBI techniqu…