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Employment (5)

Waseda University: 3-4-1 Okubo, Shinjuku, Tokyo, JP

2024-04-01 to present | Junior Researcher (Assistant Professor) (Waseda Research Institute for Science and Engineering, Faculty of Science and Engineering)
Employment
Source: Self-asserted source
Ken Mawatari

University of Tsukuba: Tsukuba, Ibaraki, JP

2023-04-01 to 2024-03-31 | Posdoc Fellow
Employment
Source: Self-asserted source
Ken Mawatari

自然科学研究機構国立天文台/National Astronomical Observatory of Japan: 三鷹市/Mitaka City/Mitaka City, 東京都/Tokyo/Tokyo, JP

2021-04-01 to 2023-03-31 | 特任研究員/Project Researcher (ハワイ観測所/Subaru Telescope)
Employment
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National Institutes of Natural Sciences

University of Tokyo: Kashiwa, Tokyo, JP

2018-04-01 to 2021-03-31 | ICRR Fellow (Institute for Cosmic Ray Research)
Employment
Source: Self-asserted source
Ken Mawatari

Osaka Sangyo University: Daito, Osaka, JP

2015-04-01 to 2018-03-31 | Postdoctoral Fellow (Department of Environmental Science and Technology)
Employment
Source: Self-asserted source
Ken Mawatari

Education and qualifications (1)

Tohoku University: Sendai, Miyagi, JP

2006-04-01 to 2015-03-27 | Ph.D (Faculty of Science)
Education
Source: Self-asserted source
Ken Mawatari

Works (13)

``Big Three Dragons'': a z = 7.15 Lyman BreakGalaxy Detected in [OIII] 88 $μ$m, [CII] 158 $μ$m, and Dust Continuum with ALMA

ArXiv e-prints
2018-06 | Journal article
Source: Self-asserted source
Ken Mawatari

Detection of the Far-infrared [O III] and Dust Emission in a Galaxy at Redshift 8.312: Early Metal Enrichment in the Heart of the Reionization Era

ArXiv e-prints
2018-06 | Journal article
Source: Self-asserted source
Ken Mawatari

CHORUS II. Subaru/HSC Determination of the Ly$α$ Luminosity Function at $z=7.0$: Constraints on Cosmic Reionization Model Parameter

ArXiv e-prints
2018-05 | Journal article
Source: Self-asserted source
Ken Mawatari

The onset of star formation 250 million years after the Big Bang

\nat
2018-05 | Journal article
DOI: 10.1038/s41586-018-0117-z
Source: Self-asserted source
Ken Mawatari

Mapping of HI Absorption Structure in the SSA22 Protocluster at z = 3.1

Early stages of Galaxy Cluster Formation
2017-07 | Conference paper
DOI: 10.5281/zenodo.832891
Source: Self-asserted source
Ken Mawatari

Imaging of diffuse H I absorption structure in the SSA22 protocluster region at z = 3.1

\mnras
2017-06 | Journal article
DOI: 10.1093/mnras/stx038
Source: Self-asserted source
Ken Mawatari

Detection of an oxygen emission line from a high-redshift galaxy in the reionization epoch

Science
2016-06 | Journal article
DOI: 10.1126/science.aaf0714
Source: Self-asserted source
Ken Mawatari

Possible identification of massive and evolved galaxies at z \gsim 5

\pasj
2016-06 | Journal article
DOI: 10.1093/pasj/psw041
Source: Self-asserted source
Ken Mawatari

Discovery of a Damped Ly$α$ Absorber at z = 3.3 along a Galaxy Sight-line in the SSA22 Field

\apj
2016-02 | Journal article
DOI: 10.3847/0004-637X/817/2/161
Source: Self-asserted source
Ken Mawatari

SPT-CL J2040-4451: An SZ-selected Galaxy Cluster at z = 1.478 with Significant Ongoing Star Formation

\apj
2014-10 | Journal article
DOI: 10.1088/0004-637X/794/1/12
Source: Self-asserted source
Ken Mawatari

Characterization of the Distribution of the Ly$α$ Emitters in the 53w002 Field at z = 2.4

\apj
2012-11 | Journal article
DOI: 10.1088/0004-637X/759/2/133
Source: Self-asserted source
Ken Mawatari

WISH for deep and wide NIR surveys

Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave
2012-09 | Conference paper
DOI: 10.1117/12.925632
Source: Self-asserted source
Ken Mawatari

An H$α$ search for overdense regions at z = 2.23

\mnras
2011-09 | Journal article
DOI: 10.1111/j.1365-2966.2011.19179.x
Source: Self-asserted source
Ken Mawatari
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