HY
Hiroto Yanagisawa
astro-ph.GAastro-ph.COastro-ph.HEBurnsDiabetic FootGangrenePressure Ulcer
On Valency
published · living versionsW_unu28bt7·v1 · currentpublished
Why a Multi-Cycle Treasury Program is Essential to Maximize JWST's Scientific Contributions to Galaxy Formation
with Genesis Community, Alice Shapley, Steven L. Finkelstein, Rachel S. Somerville +416
1 version
Preprints & journals
23 papers in the corpus · 2024–2026Can Blue UV-Bright Galaxies Drive Reionization at Cosmic Dawn? An Galaxy with at 2610.24092v1 · Yunjing Wu, Sijia Cai, Yongda Zhu et al.2026 · 0 citationsarXiv
Wound/Pressure Ulcer/Burn Guidelines (2023)-3 Guidelines for the Diagnosis and Treatment of Diabetic Skin Ulcer/Gangrene (3rd Edition).42802530 · Wound/Pressure Ulcer/Burn Guidelines Drafting Committee (Diabetic Skin Ulcer/Gangrene Group), Nakanishi, Takeshi, Ikegami, Ryuta et al.2026 · 0 citationsThe Journal of dermatology. 2026;53(10):e778-e827
SN Helios: A Multiply Imaged Type II Supernova Opening Time-Delay Cosmography beyond redshift of 32609.30440v2 · Seiji Fujimoto, Conor Larison, Justin D. R. Pierel et al.2026 · 0 citationsarXiv
ATLAS. IV. A JWST+MUSE Demographic Study of Ly Profiles in Little Red Dots2608.14534v1 · Yuta Kageura, Masami Ouchi, Hiroto Yanagisawa et al.2026 · 0 citationsarXiv
ATLAS. III. Dust Around Little Red Dots: Hydrogen Line Ratios beyond Dust-free Non-Case B Models2608.10832v2 · Tomokazu Kiyota, Masami Ouchi, Hiroto Yanagisawa et al.2026 · 0 citationsarXiv
ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs2607.26269v1 · Hiroto Yanagisawa, Masami Ouchi, Tomokazu Kiyota et al.2026 · 0 citationsarXiv
ATLAS. I. A Scaling Relation of LRDs between Broad H and Bolometric Luminosities: Enhanced Broad H Emission Relative to Low- Type 1 AGN2606.09726v2 · Hiroto Yanagisawa, Masami Ouchi, Tomokazu Kiyota et al.2026 · 0 citationsarXiv
Chemical Abundance Ratios of Nitrogen Rich Galaxies Identified at : Observational Demographics and Models2603.21570v2 · Kuria Watanabe, Masami Ouchi, Kimihiko Nakajima et al.2026 · 0 citationsarXiv
Back to Normal Again: Possible Destinies of JWST overmassive SMBHs and "Little Red Dots" in the View of Shin-Uchuu Simulation2602.14496v1 · Haojie Hu, Hiroto Yanagisawa, Moka Nishigaki et al.2026 · 1 citationarXiv
VENUS: Strong-lensing model of MACS J1931.8-2635 -- revealing the farthest multiply imaged supernova2602.14074v2 · Joseph F. V. Allingham, Adi Zitrin, Vasily Kokorev et al.2026 · 1 citationApJ 1005 215 (2026)
VENUS: Two Faint Little Red Dots Separated by Hidden in a Single Lensed Galaxy at 2601.06015v1 · Hiroto Yanagisawa, Masami Ouchi, Miriam Golubchik et al.2026 · 2 citationsarXiv
A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.132601.04156v2 · David A. Coulter, Conor Larison, Justin D. R. Pierel et al.2026 · 0 citationsarXiv
DREAMS.II. Galaxy Demographics from Direct Te-Based Metallicities at z~2-10: Tracing the Evolution of the Mass-Metallicity and Fundamental Relations2512.12983v1 · Moka Nishigaki, Kimihiko Nakajima, Masami Ouchi et al.2025 · 0 citationsarXiv
Little red dot variability over a century reveals black hole envelope via a giant Einstein cross2512.05180v1 · Zijian Zhang, Mingyu Li, Masamune Oguri et al.2025 · 2 citationsarXiv
EMPRESS. XV. A New Determination of the Primordial Helium Abundance Suggesting a Moderately Low Value2506.24050v3 · Hiroto Yanagisawa, Masami Ouchi, Akinori Matsumoto et al.2025 · 0 citationsarXiv
Fe Abundances of Early Galaxies at Derived with Deep JWST Spectra2503.11457v3 · Minami Nakane, Masami Ouchi, Kimihiko Nakajima et al.2025 · 12 citationsarXiv
EMPRESS. X. Spatially resolved mass-metallicity relation in extremely metal-poor galaxies: evidence of episodic star-formation fueled by a metal-poor gas infall2412.04541v1 · Kimihiko Nakajima, Masami Ouchi, Yuki Isobe et al.2024 · 0 citationsarXiv
A Galaxy with an Extremely Blue UV Slope at Identified by JWST Spectroscopy: Evidence for a Weak Nebular Continuum and Efficient Ionizing Photon Escape?2411.19893v3 · Hiroto Yanagisawa, Masami Ouchi, Kimihiko Nakajima et al.2024 · 1 citationarXiv
Low [O/Fe] Ratio in a Luminous Galaxy at the Early Cosmic Epoch (): Signature of Short Delay Time or Bright Hypernovae/Pair-Instability Supernovae?2407.14470v3 · Minami Nakane, Masami Ouchi, Kimihiko Nakajima et al.2024 · 8 citationsarXiv
JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z~7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe2406.18352v2 · Yuichi Harikane, Akio K. Inoue, Richard S. Ellis et al.2024 · 102 citationsarXiv
Strong He I Emission Lines in High N/O Galaxies at Identified in JWST Spectra: High He/H Abundance Ratios or High Electron Densities?2405.01823v2 · Hiroto Yanagisawa, Masami Ouchi, Kuria Watanabe et al.2024 · 2 citationsarXiv
Dynamics of a Galaxy at z > 10 Explored by JWST Integral Field Spectroscopy: Hints of Rotating Disk Suggesting Weak Feedback2404.16963v3 · Yi Xu, Masami Ouchi, Hidenobu Yajima et al.2024 · 17 citationsarXiv
Balmer Decrement Anomalies in Galaxies at z ~ 6 Found by JWST Observations: Density-Bounded Nebulae or Excited H I Clouds?2403.20118v2 · Hiroto Yanagisawa, Masami Ouchi, Kimihiko Nakajima et al.2024 · 22 citationsarXiv
Career total: 32 works. 23 are in this corpus.
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