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Disambiguation of "Shibuya, Takatoshi"

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Morphologies of Galaxies at $z 9-17$ Uncovered by JWST/NIRCam Imaging: Cosmic Size Evolution and an Identification of an Extremely Compact Bright Galaxy at $z12$

, , , , , , , , , and . (2022)cite arxiv:2208.13582Comment: 26 pages, 23 figures, submitted to ApJ.

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Rie Shibuya

Katsuhisa Shibuya

Shigeaki Shibuya

 

Other publications of authors with the same name

SILVERRUSH. XI. Intensity Mapping for Lya Emission Extending over $100-1000$ comoving kpc around $z\sim2-7$ LAEs with Subaru HSC-SSP and CHORUS Data, , , , , , , , , and 7 other author(s). (2021)cite arxiv:2108.09288.SILVERRUSH. XIII. A Catalog of 20,567 Ly$\alpha$ Emitters at $z=2-7$ Identified in the Full-depth Data of the Subaru/HSC-SSP and CHORUS Surveys, , , , , , , , , and 6 other author(s). (2023)cite arxiv:2305.08921Comment: 38 pages, 19 Figures, 5 Tables. Accepted for publication in ApJS.Ly$\alpha$ Emitters with Very Large Ly$\alpha$ Equivalent Widths, EW$_0$(Ly$\alpha$) $200-400$ \AA, at $z2$, , , , , , , , and . (2016)cite arxiv:1611.00777Comment: Accepted for publication in MNRAS; 23 pages with 16 figures.SILVERRUSH. III. Deep Optical and Near-Infrared Spectroscopy for Lya and UV-Nebular Lines of Bright Lya Emitters at z=6-7, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1705.00733Comment: 24 pages, 11 figures, submitted to PASJ special issue.3D Distribution Map of HI Gas and Galaxies Around an Enormous Ly$\alpha$ Nebula and Three QSOs at $z=2.3$ Revealed by the HI Tomographic Mapping Technique, , , , , , , , , and 15 other author(s). (2019)cite arxiv:1910.02962Comment: 14 pages, 7 figures, submitted to ApJ.Evolution of Galactic Outflows at $z\sim0$-$2$ Revealed with SDSS, DEEP2, and Keck spectra, , , , , , , and . (2017)cite arxiv:1703.01885Comment: 12 pages, 8 figures, submitted to ApJ.Diffuse Ly$\alpha$ Halos around Galaxies at $z=2.2-6.6$: Implications for Galaxy Formation and Cosmic Reionization, , , , , , , , and . (2014)cite arxiv:1403.0732Comment: 11 pages, 9 figures, 1 table. Submitted to MNRAS.A Cose Comparison between Observed and modeled Ly\alpha Lines for z ~ 2.2 Lyman Alpha Emitters, , , , , , , , , and . (2015)cite arxiv:1504.03693Comment: 26 pages, 15 figures, 6 tables, submitted to ApJ.SILVERRUSH. VI. A simulation of Ly$\alpha$ emitters in the reionization epoch and a comparison with Subaru Hyper Suprime-Cam survey early data, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1801.00067Comment: Submitted to PASJ, 29 pages, 20 figures.What is the Physical Origin of Strong Lya Emission? I. Demographics of Lya Emitter Structures, , , , , , , and . (2014)cite arxiv:1401.1209Comment: 13 pages, 15 figures, 3 tables, submitted to ApJ.