activity
20022025
most citedThe Infrared Astronomical Mission AKARI

842 citations · 2.9k across the 60 of their papers we have counts for

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Showing astro-ph.SRShow all

22 papers · 1 filter

astro-ph.SR2025

The age and metallicity dependence of the near-infrared absolute magnitude and colour of red clump stars

Hiroki Onozato, Yoshifusa Ita, Yoshikazu Nakada

Understanding the age and metallicity dependence of the absolute magnitude and colour of red clump (RC) stars is crucial for validating the accuracy of stellar evolution models and…

astro-ph.SR2022★ 1 cited

The Thirty Millimeter Telescope

Yoshifusa Ita, Takashi Ichikawa, Hironori Tsutsui +11

A near-infrared telescope with an effective aperture diameter of thirty millimeters has been developed. The primary objective of the development is to observe northern bright stars…

astro-ph.SR2022★ 8 cited

A Very Metal-poor RR Lyrae Star with a Disk Orbit Found in the Solar Neighborhood

Noriyuki Matsunaga, Akinori Itane, Kohei Hattori +28

Metal-deficient stars are important tracers for understanding the early formation of the Galaxy. Recent large-scale surveys with both photometric and spectroscopic data have report…

astro-ph.SR2020★ 11 cited

Light and colour variations of Mira variables in the Small Magellanic Cloud

Yoshifusa Ita, John W. Menzies, Patricia A. Whitelock +6

The goal of this paper is to characterise the light variation properties of Mira variables in the Small Magellanic Cloud. We have investigated a combined optical and near infrared…

astro-ph.SR2020★ 4 cited

Long-Term Near-Infrared Brightening of Non-Variable OH/IR Stars

Takafumi Kamizuka, Yoshikazu Nakada, Kenshi Yanagisawa +8

Non-variable OH/IR stars are thought to have just left the asymptotic giant branch (AGB) phase. In this conventional picture, they must still show strong circumstellar extinction c…

astro-ph.SR2019★ 11 cited

Long Secondary Periods in luminous red giant variables

Masaki Takayama, Yoshifusa Ita

The origin of long secondary periods (LSPs) in red giant variables is unknown. We investigate whether stellar pulsations in red giants can explain the properties of the LSP variabi…