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Takashi Saito

Researcher at Nagoya City University

Publications -  1220
Citations -  60014

Takashi Saito is an academic researcher from Nagoya City University. The author has contributed to research in topics: Medicine & MAGIC (telescope). The author has an hindex of 112, co-authored 1041 publications receiving 52937 citations. Previous affiliations of Takashi Saito include Mitsubishi Electric & Nippon Medical School.

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Serine Phosphorylation of IRS1 Correlates with Aβ-Unrelated Memory Deficits and Elevation in Aβ Level Prior to the Onset of Memory Decline in AD

TL;DR: The modifications of IRS1 through its phosphorylation at etiology-specific Ser sites are shown in various animal models of memory decline, such as diabetic, aged, and amyloid precursor protein (APP) knock-in NL-G-F (APPKINL-F) mice to suggest a potential marker of Aβ-unrelated memory deficits caused by type 2 diabetes and aging.
Journal Article

Dendritic Cell Differentiation and Tumor Cell Apoptosis Induced by Components of a Poly-phenylpropanoid Polysaccharide Complex

TL;DR: The effects on dendritic cells and the inhibition of tumor growth, if they occur to a significant level in vivo, could help explain the apparent usefulness of PPC in the treatment of cancer.
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MAGIC search for VHE gamma-ray emission from AE Aquarii in a multiwavelength context

Jelena Aleksić, +160 more
TL;DR: In this article, it was shown that AE Aqr is not a very high-energy (VHE, E > 100 GeV) source both on observational and theoretical grounds.
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Anomalously High Ionic Conductivity of Li2SiS3-Type Conductors.

TL;DR: Li2SiS3 as mentioned in this paper is a lithium superionic conductor with tetragonal crystal symmetry, which possesses a new three-dimensional framework structure consisting of isolated edge-sharing tetrahedral dimers.
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Very high energy gamma-ray observation of the peculiar transient event Swift J1644+57 with the MAGIC telescopes and AGILE

Jelena Aleksić, +164 more
TL;DR: The MAGIC telescopes observed the peculiar source Swift J1644+57 during the flaring phase, searching for gamma-ray emission at very-high energy (VHE, E > 100 GeV), starting observations nearly 2.5 days after the trigger time.