activity
20232026
most citedMAGIS (Measuring Abundances of red super Giants with Infrared Spectroscopy) project I. Establishment of an abundance analysis procedure for red supergiants and its evaluation with nearby stars

8 citations · 13 across the 12 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2026

He I 10830 Resonant Scattering in M17: Toward a Diagnostic of Optical Depth and Gas Kinematics

Hiroaki Sameshima, Daisuke Taniguchi, Noriyuki Matsunaga +2

The lower level of the He I 10830 transition is metastable and therefore well populated. In H II regions, the line can become optically thick, and its photons then undergo reson…

astro-ph.GA2026

Impact of Gaia-Sausage-Enceladus merger revealed by a single cosmic clock: thick-to-thin disc transition, gas disc shrinking and bar formation

Natsuki Funakoshi, Daisuke Kawata, Jason L. Sanders +5

Whether the formation of the Galactic bar was connected to the Gaia-Sausage-Enceladus (GSE) merger, the last significant merger experienced by the Milky Way, remains an open questi…

astro-ph.GA2026

Kinematical and dynamical properties of recently discovered bulge and disc star clusters with WINERED

Ilaria Petralia, Dante Minniti, José G. Fernández-Trincado +8

Context. Galactic globular clusters are a very important tool in explaining the characteristics of the Milky Way. Therefore it is essential to determine the kinematical and dynamic…

astro-ph.EP2025★ 1 cited

First Results from WINERED: Detection of Emission Lines from Neutral Iron and a Combined Set of Trace Species on the Dayside of WASP-189 b

Lennart van Sluijs, Emily Rauscher, Eliza M. -R. Kempton +9

Ground and space-based observations have revealed that Ultra Hot Jupiters (UHJs,~) typically have inverted thermal profiles, while cooler hot Jupiters…

astro-ph.EP2025★ 1 cited

Assessing robustness and bias in 1D retrievals of 3D Global Circulation Models at high spectral resolution: a WASP-76 b simulation case study in emission

Lennart van Sluijs, Hayley Beltz, Isaac Malsky +4

High-resolution spectroscopy (HRS) of exoplanet atmospheres has successfully detected many chemical species and is quickly moving toward detailed characterization of the chemical a…

astro-ph.GA2025

Discovery of WINERED-HVS1: A metal-rich hyper-velocity star candidate ejected from the Galactic center

Kohei Hattori, Daisuke Taniguchi, Takuji Tsujimoto +4

We report the discovery of a metal-rich red giant star, WINERED-HVS1, which is a candidate for a hyper-velocity star (HVS). Its past trajectory suggests that this star may have bee…

astro-ph.GA2025★ 8 cited

MAGIS (Measuring Abundances of red super Giants with Infrared Spectroscopy) project I. Establishment of an abundance analysis procedure for red supergiants and its evaluation with nearby stars

Daisuke Taniguchi, Noriyuki Matsunaga, Naoto Kobayashi +11

[Abbreviated] Context. Given their high luminosities (L>~10^4Lsun), red supergiants (RSGs) are good tracers of the chemical abundances of the young stellar population in the Milky…

astro-ph.EP2024

[N I] 10400/10410 Å Lines as Possible Disk Wind Tracers in a Young Intermediate-Mass Star

Haruki Katoh, Chikako Yasui, Yuji Ikeda +10

In this study, we performed high-resolution near-infrared (NIR) spectroscopy (R = 28,000; -1.35 m) with a high signal-to-noise ratio on HD 200775, a very young (${\sim…

astro-ph.CO2024★ 1 cited

First Result for Dark Matter Search by WINERED

Wen Yin, Taiki Bessho, Yuji Ikeda +10

The identity of dark matter has been a mystery in astronomy, cosmology, and particle theory for about a century. Bessho, Ikeda, and Yin (2022), three of the current authors, propos…

astro-ph.EP2024

A High-Resolution Non-Detection of Escaping Helium In The Ultra-Hot Neptune LTT 9779b: Evidence for Weakened Evaporation

Shreyas Vissapragada, Patrick McCreery, Leonardo A. Dos Santos +16

The recent discovery of ``ultra-hot'' ( day) Neptunes has come as a surprise: some of these planets have managed to retain gaseous envelopes despite being close enough to th…

astro-ph.IM2024

WARP: The Data Reduction Pipeline for the WINERED spectrograph

Satoshi Hamano, Yuji Ikeda, Shogo Otsubo +8

We present a data reduction pipeline written in Python for data obtained with the near-infrared cross-dispersed echelle spectrograph, WINERED, which yields a 0.911.35 m spect…

astro-ph.GA2024

Clues to growth and disruption of two neighbouring spiral arms of the Milky Way

Natsuki Funakoshi, Noriyuki Matsunaga, Daisuke Kawata +3

Studying the nature of spiral arms is essential for understanding the formation of the intricate disc structure of the Milky Way. The European Space Agency's Gaia mission has provi…

astro-ph.GA2023

The globular cluster VVV CL002 falling down to the hazardous Galactic centre

D. Minniti, N. Matsunaga, J. G. Fernandez-Trincado +15

Context. The Galactic centre is hazardous for stellar clusters because of the strong tidal force. Supposedly, many clusters were destroyed and contributed stars to the crowded stel…

astro-ph.GA2023★ 2 cited

The epoch of the Milky Way's bar formation: dynamical modelling of Mira variables in the nuclear stellar disc

Jason L. Sanders, Daisuke Kawata, Noriyuki Matsunaga +4

A key event in the history of the Milky Way is the formation of the bar. This event affects the subsequent structural and dynamical evolution of the entire Galaxy. When the bar for…