HS
Hiroaki Sameshima
astro-ph.GAastro-ph.SRastro-ph.COastro-ph.HEastro-ph.IMastro-ph.EPastro-phhep-ph
On Valency
published · living versionsW_vr64scbx·v1 · currentpublished
He I 10830 Resonant Scattering in M17: Toward a Diagnostic of Optical Depth and Gas Kinematics
with Daisuke Taniguchi, Noriyuki Matsunaga, Shogo Otsubo, Tomomi Takeuchi
1 version
Preprints & journals
51 papers in the corpus · 2008–2026Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP2608.10074v1 · Ayumi Takahashi, Yoshiki Matsuoka, Yoshiki Toba et al.2026 · 0 citationsarXiv
High-Precision Near-Infrared Abundances of Solar Analogs in the YJ Bands2604.00981v1 · Noriyuki Matsunaga, Takuji Tsujimoto, Daisuke Taniguchi et al.2026 · 1 citationarXiv
Kinematical and dynamical properties of recently discovered bulge and disc star clusters with WINERED2603.15450v1 · Ilaria Petralia, Dante Minniti, Jos'e G. Fern'andez-Trincado et al.2026 · 0 citationsarXiv
Diverse Origins of Broad H Lines in Heavily Obscured AGNs Revealed by Multi-epoch Spectroscopy2601.08212v1 · Shoichiro Mizukoshi, Takeo Minezaki, Subaru Ubukata et al.2026 · 0 citationsarXiv
Discovery of WINERED-HVS1: A metal-rich hyper-velocity star candidate ejected from the Galactic center2502.20266v2 · Kohei Hattori, Daisuke Taniguchi, Takuji Tsujimoto et al.2025 · 4 citationsarXiv
First Result for Dark Matter Search by WINERED.39983159 · Yin, Wen, Bessho, Taiki, Ikeda, Yuji et al.2025 · 21 citationsPhysical review letters. 2025;134(5):051004
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 stars2501.10502v1 · Daisuke Taniguchi, Noriyuki Matsunaga, Naoto Kobayashi et al.2025 · 8 citationsA&A, 693, A163 (2025)
Updated Picture of the Active Galactic Nuclei with Dusty/Dust-free Gas Structures and Effects of the Radiation Pressure2406.08720v1 · Shoichiro Mizukoshi, Takeo Minezaki, Hiroaki Sameshima et al.2024 · 6 citationsarXiv
X-ray Winds In Nearby-to-distant Galaxies (X-WING) - I: Legacy Surveys of Galaxies with Ultrafast Outflows and Warm Absorbers in -2405.02391v1 · Satoshi Yamada, Taiki Kawamuro, Misaki Mizumoto et al.2024 · 1 citationarXiv
[N I] 10400/10410 Å Lines as Possible Disk Wind Tracers in a Young Intermediate-Mass Star2403.09774v1 · Haruki Katoh, Chikako Yasui, Yuji Ikeda et al.2024 · 1 citationarXiv
WARP: The Data Reduction Pipeline for the WINERED spectrograph2401.04876v1 · Satoshi Hamano, Yuji Ikeda, Shogo Otsubo et al.2024 · 10 citationsarXiv
Shock Excitation in Narrow Line Regions Powered by AGN Outflows2311.13085v1 · Misaki Mizumoto, Hiroaki Sameshima, Naoto Kobayashi et al.2023 · 3 citationsarXiv
Astrophysical calibration of the oscillator strengths of YJ-band absorption lines in classical Cepheids2307.00158v1 · S. S. Elgueta, N. Matsunaga, M. Jian et al.2023 · 7 citationsarXiv
Quasar Luminosity Function at z = 72305.11225v1 · Yoshiki Matsuoka, Masafusa Onoue, Kazushi Iwasawa et al.2023 · 66 citationsarXiv
Narrow Fe-K Reverberation Mapping Unveils the Deactivated Broad-Line Region in a Changing-Look Active Galactic Nucleus2212.02731v1 · Hirofumi Noda, Taisei Mineta, Takeo Minezaki et al.2022 · 19 citationsarXiv
Measurement of AGN dust extinction based on the near-infrared flux variability of WISE data2209.07933v1 · Shoichiro Mizukoshi, Takeo Minezaki, Shoichi Tsunetsugu et al.2022 · 9 citationsMNRAS, 516, 2876 (2022)
Potential signature of Population III pair-instability supernova ejecta in the BLR gas of the most distant quasar at z = 7.542207.11909v1 · Yuzuru Yoshii, Hiroaki Sameshima, Takuji Tsujimoto et al.2022 · 21 citationsarXiv
Survey of near-infrared diffuse interstellar bands in and bands. I. Newly identified bands2206.03131v3 · Satoshi Hamano, Naoto Kobayashi, Hideyo Kawakita et al.2022 · 18 citationsarXiv
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.02111.12766v1 · Yoshiki Matsuoka, Kazushi Iwasawa, Masafusa Onoue et al.2021 · 61 citationsarXiv
Effective temperatures of red supergiants estimated from line-depth ratios of iron lines in the YJ bands, 0.97--1.32 micron2012.07856v3 · Daisuke Taniguchi, Noriyuki Matsunaga, Mingjie Jian et al.2020 · 22 citationsMNRAS, 502, 4210 (2021); Erratum: MNRAS, 512, 2669 (2022)
The effect of surface gravity on line-depth ratios in the wavelength range 0.97-1.32 {\mu}m2003.10641v2 · Mingjie Jian, Daisuke Taniguchi, Noriyuki Matsunaga et al.2020 · 10 citationsarXiv
Identification of Absorption Lines of Heavy Metals in the Wavelength Range 0.97--1.32 Micron1911.11277v1 · Noriyuki Matsunaga, Daisuke Taniguchi, Mingjie Jian et al.2019 · 16 citationsarXiv
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). X. Discovery of 35 Quasars and Luminous Galaxies at 5.7 z 7.01908.07910v1 · Yoshiki Matsuoka, Kazushi Iwasawa, Masafusa Onoue et al.2019 · 128 citationsApJ 883:183, 2019
WINERED high-resolution near-infrared line catalog: A-type star1810.07206v1 · H. Sameshima, Y. Ikeda, N. Matsunaga et al.2018 · 2 citationsarXiv
A newly-identified emission-line region around P Cygni1808.04622v1 · Misaki Mizumoto, Naoto Kobayashi, Satoshi Hamano et al.2018 · 5 citationsarXiv
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). IV. Discovery of 41 Quasars and Luminous Galaxies at 5.7 < z < 6.91803.01861v2 · Y. Matsuoka, K. Iwasawa, M. Onoue et al.2018 · 132 citationsApJS 237 (2018) 5
On the chemical abundances of Miras in clusters: V1 in the metal-rich globular NGC 59271802.07314v1 · V. D'Orazi, D. Magurno, G. Bono et al.2018 · 11 citationsarXiv
Method to Estimate the Effective Temperatures of Late-Type Giants using Line-Depth Ratios in the Wavelength Range 0.97-1.32$\mu $m1710.04674v1 · Daisuke Taniguchi, Noriyuki Matsunaga, Naoto Kobayashi et al.2017 · 23 citationsarXiv
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). II. Discovery of 32 Quasars and Luminous Galaxies at 5.7 < z < 6.81704.05854v3 · Yoshiki Matsuoka, Masafusa Onoue, Nobunari Kashikawa et al.2017 · 140 citationsPASJ 70 (2018) 35
Ultraviolet to optical diffuse sky emission as seen by the Hubble Space Telescope Faint Object Spectrograph1701.00885v1 · K. Kawara, Y. Matsuoka, K. Sano et al.2017 · 47 citationsarXiv
Chemical evolution of the Universe at 0.7 < z < 1.6 derived from abundance diagnostics of the broad-line region of quasars1611.06027v1 · Hiroaki Sameshima, Yuzuru Yoshii, Kimiaki Kawara2016 · 31 citationsarXiv
Hitomi constraints on the 3.5 keV line in the Perseus galaxy cluster1607.07420v2 · Felix A. Aharonian, Hiroki Akamatsu, Fumie Akimoto et al.2016 · 122 citationsApJ, 837, L15 (2017)
The Quiescent Intracluster Medium in the Core of the Perseus Cluster1607.04487v1 · Felix Aharonian, Hiroki Akamatsu, Fumie Akimoto et al.2016 · 493 citationsarXiv
Origin of the Characteristic X-ray Spectral Variations of IRAS 13224$-$38091607.00879v1 · Hiroki Yamasaki, Misaki Mizumoto, Ken Ebisawa et al.2016 · 14 citationsarXiv
Subaru high-z exploration of low-luminosity quasars (SHELLQs). I. Discovery of 15 quasars and bright galaxies at 5.7 < z < 6.91603.02281v3 · Yoshiki Matsuoka, Masafusa Onoue, Nobunari Kashikawa et al.2016 · 228 citationsApJ 828 (2016) 26
Near infrared diffuse interstellar bands toward the Cygnus OB2 association1602.06959v1 · Satoshi Hamano, Naoto Kobayashi, Sohei Kondo et al.2016 · 40 citationsarXiv
Origin of the Broad Iron Line Feature and the Soft X-ray Variation in Seyfert Galaxies1602.04284v1 · Naoki Iso, Ken Ebisawa, Hiroaki Sameshima et al.2016 · 21 citationsarXiv
Observations of Gamma-ray Bursts with ASTRO-H and Fermi1503.01182v1 · M. Ohno, T. Kawano, M. S. Tashiro et al.2015 · 0 citationsarXiv
ASTRO-H White Paper - AGN Winds1412.1171v1 · J. S. Kaastra (SRON), Y. Terashima, T. Kallman (NASA/GSFC) et al.2014 · 4 citationsarXiv
ASTRO-H White Paper - Chemical Evolution in High-z Universe1412.1179v1 · M. S. Tashiro, D. Yonetoku, M. Ohno et al.2014 · 1 citationarXiv
The ASTRO-H X-ray Astronomy Satellite1412.1356v1 · Tadayuki Takahashi, Kazuhisa Mitsuda, Richard Kelley et al.2014 · 54 citationsarXiv
Interpretation of the X-ray Spectral Variation of 1H0707-495 with a Variable Double Partial Covering Model1409.3019v1 · Misaki Mizumoto, Ken Ebisawa, Hiroaki Sameshima2014 · 26 citationsarXiv
Statistical Properties of Multi-epoch Spectral Variability of SDSS Stripe82 Quasars1401.5074v2 · Mitsuru Kokubo, Tomoki Morokuma, Takeo Minezaki et al.2014 · 45 citationsThe Astrophysical Journal 783 (2014) 46
Diffuse Galactic Light in the Field of the Translucent High Galactic Latitude Cloud MBM321303.0938v1 · N. Ienaka, K. Kawara, Y. Matsuoka et al.2013 · 43 citationsarXiv
The ASTRO-H X-ray Observatory1210.4378v1 · Tadayuki Takahashi, Kazuhisa Mitsuda, Richard Kelley et al.2012 · 110 citationsarXiv
Extinction law in ultraluminous infrared galaxies at z ~ 11107.5381v1 · T. Shimizu, K. Kawara, H. Sameshima et al.2011 · 7 citationsarXiv
Ultraviolet Continuum Color Variability of Luminous Sloan Digital Sky Survey QSOs1103.3619v1 · Yu Sakata, Tomoki Morokuma, Takeo Minezaki et al.2011 · 37 citationsarXiv
Supernova dust for the extinction law in a young infrared galaxy at z = 11011.0511v1 · K. Kawara, H. Hirashita, T. Nozawa et al.2010 · 2 citationsarXiv
Implications from the optical to UV flux ratio of FeII emission in quasars1008.2405v1 · H.Sameshima, K.Kawara, Y.Matsuoka et al.2010 · 27 citationsarXiv
Stellar population and dust extinction in an ultraluminous infrared galaxy at z=1.1350910.2792v2 · K. Kawara, S. Oyabu, Y. Matsuoka et al.2009 · 8 citationsarXiv
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