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Kazuaki Ota

Researcher at University of Tokyo

Publications -  44
Citations -  5580

Kazuaki Ota is an academic researcher from University of Tokyo. The author has contributed to research in topics: Galaxy & Hubble Deep Field. The author has an hindex of 30, co-authored 43 publications receiving 5429 citations. Previous affiliations of Kazuaki Ota include Max Planck Society.

Papers
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STATISTICS OF 207 Lyα EMITTERS AT A REDSHIFT NEAR 7: CONSTRAINTS ON REIONIZATION AND GALAXY FORMATION MODELS*

TL;DR: In this paper, the authors presented the Ly{alpha} luminosity function (LF), clustering measurements, and Ly{α} line profiles based on the largest sample to date of 207 Lyα emitters (LAEs) at z = 6.6 on the 1 deg{sup 2} sky of Subaru/XMM-Newton Deep Survey field.
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Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation Models

TL;DR: In this paper, the authors presented Lya luminosity function (LF), clustering measurements, and Lya line profiles based on the largest sample, to date, of 207 Lya emitters (LAEs) at z=6.6 on the 1-deg^2 sky of Subaru/XMM-Newton Deep Survey (SXDS) field.
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Subaru Deep Survey V. A Census of Lyman Break Galaxies at z=4 and 5 in the Subaru Deep Fields: Photometric Properties

TL;DR: In this paper, photometric properties of Lyman Break Galaxies (LBGs) at z=3.5-5.2 were investigated based on large samples of 2,600 LBGs detected in deep (i'~27) and wide-field (1,200 arcmin^2) images taken in the Subaru Deep Field and the Subaru/XMM Deep Field (SXDF).
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Subaru Deep Survey. VI. A Census of Lyman Break Galaxies at z ≃ 4 and 5 in the Subaru Deep Fields: Clustering Properties*

TL;DR: In this article, the photometric properties of Lyman break galaxies (LBGs) at z = 3.5-5.2 were investigated based on large samples of 2600 LBGs detected in deep (i' 27) and wide-field (1200 arcmin2) images taken in the Subaru Deep Field (SDF) and the XMM-Newton deep field (SXDF) using broadband B, V, R, i', and z' filters.
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A galaxy at a redshift z = 6.96

TL;DR: A spectroscopic redshift of z = 6.96 is reported for a galaxy whose spectrum clearly shows Lyman-α emission at 9,682 Å, indicating active star formation at a rate of ∼10M[circdot] yr-1, which demonstrates that galaxy formation was under way when the Universe was only ∼6 per cent of its present age.