output
19972026
most citedThe Infrared Astronomical Mission AKARI

842 citations

101 papers

astro-ph.SR2026

Detection of Doppler velocity differences between ions and neutrals in an erupting prominence

Yuwei Huang, Kiyoshi Ichimoto, Tetsu Anan

We performed a spectroscopic observation of an erupting prominence occurred on the solar limb on 2015 May 8th in He I 706.5 nm, O I 777.2 nm triplet and Ca II 849.8 nm lines to inv…

astro-ph.SR2026★ 10 cited

The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III

Y. Katsukawa, J. C. del Toro Iniesta, S. K. Solanki +54

The Sunrise balloon-borne solar observatory is equipped with a one-meter aperture optical telescope, offering a unique platform for uninterrupted seeing-free observations across ul…

astro-ph.EP2024★ 7 cited

Diffraction modelling of a 2023 March 5 stellar occultation by subkilometer-sized asteroid (98943) 2001 CC21

Ko Arimatsu, Fumi Yoshida, Tsutomu Hayamizu +31

We present an analysis of a stellar occultation event caused by a near-Earth asteroid (98943) 2001 CC21, an upcoming flyby target in the Hayabusa2 extended mission, on March 5, 202…

astro-ph.SR2022★ 7 cited

Spectroscopic Observations of V455 Andromedae Superoutburst in 2007: the Most Exotic Spectral Features in Dwarf Nova Outbursts

Yusuke Tampo, Daisaku Nogami, Taichi Kato +10

We present our spectroscopic observations of V455 Andromedae during the 2007 superoutburst. Our observations cover this superoutburst from around the optical peak of the outburst t…

astro-ph.SR2020★ 1 cited

Spectrum variability of the active solar-type star Xi Bootis A

Yoichi Takeda, Satoshi Honda, Hikaru Taguchi +1

An extensive spectroscopic study on ξBoo A (chromospherically active solar-type star) was conducted based on the spectra obtained in 2008 December though 2010 May, with an aim to d…

astro-ph.SR2018★ 6 cited

Spectroscopic Determination of Capella's Photospheric Abundances: Possible Influence of Stellar Activity

Yoichi Takeda, Osamu Hashimoto, Satoshi Honda

Capella is a spectroscopic binary consisting of two G-type giants, where the primary (G8III) is a normal red-clump giant while the secondary (G0III) is a chromospherically-active f…