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Takashi J. Moriya

Researcher at National Institutes of Natural Sciences, Japan

Publications -  254
Citations -  7840

Takashi J. Moriya is an academic researcher from National Institutes of Natural Sciences, Japan. The author has contributed to research in topics: Supernova & Light curve. The author has an hindex of 43, co-authored 221 publications receiving 6495 citations. Previous affiliations of Takashi J. Moriya include University of Bonn & Monash University.

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Journal ArticleDOI

Euclid: Searching for pair-instability supernovae with the Deep Survey

Takashi J. Moriya, +372 more
TL;DR: The Euclid Deep Survey is planned to make regular observations of three Euclid deep fields (40 deg2 in total) spanning the Euclid's 6-year primary mission period as discussed by the authors .
Journal ArticleDOI

Search for Thermal X-ray Features from the Crab nebula with Hitomi Soft X-ray Spectrometer

Felix Aharonian, +193 more
TL;DR: In this article, a new upper bound was obtained for the X-ray plasma mass of <~ 1Mo for a wide range of assumed shell radius, size, and plasma temperature both in and out of the collisional equilibrium.
Book ChapterDOI

Preparation of Photo-Cross-Linked Small Molecule Affinity Matrices for Affinity Selection of Protein Targets for Biologically Active Small Molecules

TL;DR: This work describes a photo-cross-linking technique to immobilize biologically active small molecules for protein target screening, without the need for chemical derivatization.
Posted Content

Low Energy Population III Supernovae and the Origin of the Extremely Metal-Poor Star SMSS J031300.36-670839.3

TL;DR: In this article, the authors performed two-dimensional numerical simulations of two low-energy Pop III supernovae, a 12.4Msun explosion and a 60 Msun explosion, and found that they have elemental yields that are a good fit to those measured in the most iron-poor star discovered to date, SMSS J031300.
Journal ArticleDOI

Extremely energetic supernova explosions embedded in a massive circumstellar medium: the case of SN 2016aps

TL;DR: In this paper, the authors performed one-dimensional radiation-hydrodynamic simulations of supernova ejecta colliding with a massive circumstellar medium (CSM) aiming at explaining SN 2016aps, likely the brightest supernova observed to date.