The relationship between the voting behavior and the political interests and sense of political efficacy among Japanese teenage voters : Survey of undergraduate students in the 2016 national election

The present study aimed to examine the relationship between the voting behavior of Japanese teenage voters and their political interests and sense of political efficacy. 225 undergraduate students, aged 18 to 19 years old, were asked to answer the questionnaire which included an item concerning participation in voting in the 2016 national elections, 8 items concerning political interests, and 8 items concerning sense of political efficacy. Comparing the scores on the subscales on political interests and political efficacy between those who voted and did not vote, a significant difference was found on the subscales on political interests, but not on political efficacy. Those who voted were more interested in both “political issue” and “political information” than those who did not vote. Results suggested that the political participation of teenage voters could be promoted by enhancing their political interests

Sensitive and rapid detection of cholera toxin-producing Vibrio cholerae using a loop-mediated isothermal amplification

<p>Abstract</p> <p>Background</p> <p><it>Vibrio cholerae </it>is widely acknowledged as one of the most important waterborne pathogen causing gastrointestinal disorders. Cholera toxin (CT) is a major virulence determinant of <it>V. cholerae</it>. Detection of CT-producing <it>V. cholerae </it>using conventional culture-, biochemical- and immunological-based assays is time-consuming and laborious, requiring more than three days. Thus, we developed a novel and highly specific loop-mediated isothermal amplification (LAMP) assay for the sensitive and rapid detection of cholera toxin (CT)-producing <it>Vibrio cholerae</it>.</p> <p>Results</p> <p>The assay provided markedly more sensitive and rapid detection of CT-producing <it>V. cholerae </it>strains than conventional biochemical and PCR assays. The assay correctly identified 34 CT-producing <it>V. cholerae </it>strains, but did not detect 13 CT non-producing <it>V. cholerae </it>and 53 non-<it>V. cholerae </it>strains. Sensitivity of the LAMP assay for direct detection of CT-producing <it>V. cholerae </it>in spiked human feces was 7.8 × 10²CFU per g (1.4 CFU per reaction). The sensitivity of the LAMP assay was 10-fold more sensitive than that of the conventional PCR assay. The LAMP assay for detection of CT-producing <it>V. cholerae </it>required less than 35 min with a single colony on thiosulfate citrate bile salt sucrose (TCBS) agar and 70 min with human feces from the beginning of DNA extraction to final determination.</p> <p>Conclusion</p> <p>The LAMP assay is a sensitive, rapid and simple tool for the detection of CT-producing <it>V. cholerae </it>and will be useful in facilitating the early diagnosis of human <it>V. cholerae </it>infection.</p

Superwind-Driven Intense H_2 Emission in NGC 6240

We have performed a long-slit K band spectroscopic observation of the luminous infrared galaxy NGC 6240. The peak position of the H_2 v=1-0 S(1) emission in the slit is located ~0.3" - 0.4" north of the southern nucleus. It is almost the midpoint between the southern nucleus and the peak position of the ^12CO J=1-0 emission. Based on the line-ratio analyses, we suggest the excitation mechanism of H_2 is pure thermal at most positions. In the southern region we find the following three velocity components in the H_2 emission: the blueshifted shell component (~-250 km s^-1 with respect to V_sys) which is recognized as a distinct C-shape distortion in the velocity field around the southern nucleus, the high-velocity blueshifted ``wing'' component (~-1000 km s^-1 with respect to V_sys), and the component indicating possible line splitting of ~500 km s^-1. The latter two components are extended to the south from the southern nucleus. We show that the kinematic properties of these three components can be reproduced by expanding motion of a shell-like structure around the southern nucleus. The offset peak position of the H_2 emission can be understood if we assume that the shell expanding to the north interacts with the extragalactic molecular gas. At the interface between the shell and the molecular gas concentration the cloud-crushing mechanism proposed by Cowie et al. (1981) may work efficiently, and the intense H_2 emission is thus expected there. All these findings lead us to propose a model that the most H_2 emission is attributed to the shock excitation driven by the superwind activity of the southern nucleus.Comment: 33 pages, 9 figures, accepted for publication in PAS

Infrared Imaging of z=2.43 Radio Galaxy B3 0731+438 with the Subaru Telescope - Detection of Hα\alpha Ionization Cones of a Powerful Radio Galaxy

We report on infrared imaging observations of the z=2.429 radio galaxy B3 0731+438 with the Subaru telescope. The images were taken with the K'-band filter and the 2.25 um narrow-band filter to examine the structure and properties of the Ha+[N II] 6548,6583 emission-line components. The Ha+[N II] emission-line image shows biconical lobes with an extent of 40 kpc, which are aligned with the radio axis. The rest-frame equivalent widths of the emission lines at these cones are as large as 1100 AA, and can be well explained by a gas-cloud model photoionized by power-law continuum radiation. The isotropic ionizing photon luminosity necessary to ionize the hydrogen gas in these cones amounts to 1e57(photons/s), which is larger than that in the majority of radio-loud QSOs. From these results, we propose that the Ha alignment effect in this object is produced by biconical gas clouds, which are swept up by the passage of radio jets, and are ionized by strong UV radiation from a hidden AGN. The continuum image consists of two components, a stellar-like point source and an extended diffuse galaxy. These are supposed to be a type-2 AGN and its host galaxy. The SED is fitted by a combination of spectra of a reddened dust-scattered AGN and an instantaneous starburst population of 500 Myr old. The stellar mass of the galaxy is estimated to be 3e11 M_solar, which is as large as that of typical 3C radio galaxies at z=1.Comment: 12 pages, 4 Postscript figures, uses PASJ2.sty, PASJ95.sty, PASJadd.sty. Accepted for publication in PASJ (2000

Perampanel Inhibits α‐Synuclein Transmission in Parkinson's Disease Models

パーキンソン病モデルへのペランパネルの有効性を確認 --パーキンソン病の進行抑制治療への期待--. 京都大学プレスリリース. 2021-04-05.[Background]: The intercellular transmission of pathogenic proteins plays a key role in the clinicopathological progression of neurodegenerative diseases. Previous studies have demonstrated that this uptake and release process is regulated by neuronal activity. [Objective]: The objective of this study was to examine the effect of perampanel, an antiepileptic drug, on α‐synuclein transmission in cultured cells and mouse models of Parkinson's disease.Methods: Mouse primary hippocampal neurons were transduced with α‐synuclein preformed fibrils to examine the effect of perampanel on the development of α‐synuclein pathology and its mechanisms of action. An α‐synuclein preformed fibril‐injected mouse model was used to validate the effect of oral administration of perampanel on the α‐synuclein pathology in vivo. [Results]: Perampanel inhibited the development of α‐synuclein pathology in mouse hippocampal neurons transduced with α‐synuclein preformed fibrils. Interestingly, perampanel blocked the neuronal uptake of α‐synuclein preformed fibrils by inhibiting macropinocytosis in a neuronal activity‐dependent manner. We confirmed that oral administration of perampanel ameliorated the development of α‐synuclein pathology in wild‐type mice inoculated with α‐synuclein preformed fibrils.[Conclusion]: Modulation of neuronal activity could be a promising therapeutic target for Parkinson's disease, and perampanel could be a novel disease‐modifying drug for Parkinson's disease

Dusty ERO Search behind Two Massive Clusters

We performed deep K'-band imaging observations of 2 massive clusters, MS 0451.6-0305 at z = 0.55 and MS 0440.5+0204 at z = 0.19, for searching counterparts of the faint sub-mm sources behind these clusters, which would provide one of the deepest extremely red object(ERO) samples. Comparing our near-infrared images with optical images taken by the Hubble Space Telescope and by the Subaru Telescope, we identified 13 EROs in these fields. The sky distributions of EROs are consistent with the previous results, that there is a sign of strong clustering among detected EROs. Also, the surface density with corrected lensing amplification factors in both clusters are in good agreement with that derived from previous surveys. We found 7 EROs and 3 additional very red objects in a small area (\sim 0.6 arcmin^2) of the MS 0451.6-0305 field around an extended SCUBA source. Many of their optical and near-infrared colors are consistent with dusty star-forming galaxies at high redshifts(z \sim 1.0-4.0), and they may be constituting a cluster of dusty starburst galaxies and/or lensed star-forming galaxies at high redshift. Their red J-K' colors and faint optical magnitudes suggest they are relatively old massive stellar systems with ages(>300 Mega years) suffering from dust obscuration. We also found a surface-density enhancement of EROs around the SCUBA source in the MS 0440.5+0204 field.Comment: 19 pages, 11 figures, Latex(using pasj00.cls). To be published in PASJ vol 55, No. 4(Aug 2003