Publications by authors named "N Kawasaki"

Severe oral mucositis is a major cause of a low quality of life in patients; however, the therapeutic effect of traditional treatments is insufficient. Therefore, we designed a carbopol gel based on rebamipide nanocrystals (REB NCs) and gum arabic (GA-REB@NP), and investigated its efficacy in accelerating wound healing in a hamster model of oral mucositis. REB NCs were prepared by bead milling, and GA- REB@NP were prepared by incorporating REB NCs into a carbopol gel.

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Siglec-7, an inhibitory receptor expressed on natural killer (NK) cells, recognizes sialic acid-containing glycans. However, the ligand glycan structures of Siglec-7 and its carrier proteins have not been comprehensively investigated. Here, we identified four sialyltransferases that are used for the synthesis of ligand glycans of Siglec-7 and two ligand O-glycan-carrier proteins, PODXL and MUC13, using a colon cancer line.

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Genome-wide association studies of primary sclerosing cholangitis have identified 23 susceptibility loci. The majority of these loci reside in non-coding regions of the genome and are thought to exert their effect by perturbing the regulation of nearby genes. Here, we aim to identify these genes to improve the biological understanding of primary sclerosing cholangitis, and nominate potential drug targets.

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Article Synopsis
  • Phosphorus binders can be combined for better effects, but their performance might change due to pH levels or other medications.
  • A study assessed how well different phosphorus binders work together, specifically looking at precipitated calcium carbonate (CC), ferric citrate hydrate (FC), lanthanum carbonate hydrate (LC), and sucroferric oxyhydroxide (SO).
  • Results showed that SO maintained a strong adsorption capacity even when mixed with other binders, while combinations of CC + FC and FC + LC had decreased effectiveness due to citrate ions interfering with calcium and lanthanum ions.*
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The isotopic compositions of samples returned from Cb-type asteroid Ryugu and Ivuna-type (CI) chondrites are distinct from other carbonaceous chondrites, which has led to the suggestion that Ryugu/CI chondrites formed in a different region of the accretion disk, possibly around the orbits of Uranus and Neptune. We show that, like for Fe, Ryugu and CI chondrites also have indistinguishable Ni isotope anomalies, which differ from those of other carbonaceous chondrites. We propose that this unique Fe and Ni isotopic composition reflects different accretion efficiencies of small FeNi metal grains among the carbonaceous chondrite parent bodies.

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