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Yuu Niino

Researcher at University of Tokyo

Publications -  73
Citations -  2051

Yuu Niino is an academic researcher from University of Tokyo. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 22, co-authored 67 publications receiving 1851 citations. Previous affiliations of Yuu Niino include National Institutes of Natural Sciences, Japan & Kyoto University.

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The host galaxy of a fast radio burst

TL;DR: The discovery of a fast radio burst is reported and the identification of a fading radio transient lasting ~6 days after the event, which is used to identify the host galaxy and measure the galaxy’s redshift, which provides a direct measurement of the cosmic density of ionized baryons in the intergalactic medium.
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The SUrvey for Pulsars and Extragalactic Radio Bursts – II. New FRB discoveries and their follow-up.

Shivani Bhandari, +191 more
TL;DR: In this article, the authors report the discovery of four fast radio bursts (FRBs) in the ongoing SUrvey for Pulsars and Extragalactic Radio Bursts at the Parkes Radio Telescope.
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Extragalactic Background Light from Hierarchical Galaxy Formation: Gamma-Ray Attenuation up to the Epoch of Cosmic Reionization and the First Stars

TL;DR: Yinoue et al. as discussed by the authors proposed a semi-analytical model of hierarchical galaxy formation that reproduces key observed properties of galaxies at various redshifts, including the potential contribution from Population III stars and following the cosmic reionization history.
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THE SUBARU HIGH-z QUASAR SURVEY: DISCOVERY OF FAINT z ∼ 6 QUASARS

TL;DR: In this paper, the authors presented the discovery of one or two extremely faint z ~ 6 quasars in 65 deg2 utilizing a unique capability of the wide-field imaging of the Subaru/Suprime-Cam.
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A SYSTEMATIC SURVEY OF PROTOCLUSTERS AT z ∼ 3–6 IN THE CFHTLS DEEP FIELDS

TL;DR: Toshikawa et al. as discussed by the authors investigated the projected sky distribution of z ∼ 3-6 Lyman-break galaxies and identified 21 protocluster candidates from regions that are overdense at more than 4σ overdensity significance.