82 research outputs found

    MicroRNA-320a inhibits cell proliferation, migration and invasion by targeting BMI-1 in nasopharyngeal carcinoma

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    AbstractIn the present study, we investigated the roles and molecular mechanisms of miR-320a in human nasopharyngeal carcinoma (NPC). miR-320a expression was strongly reduced in NPC tissues and cell lines. Overexpression of miR-320a significantly suppressed NPC cell growth, migration, invasion and tumor growth in a xenograft mouse model. A luciferase reporter assay revealed that miR-320a could directly bind to the 3′ UTR of BMI-1. Overexpression of BMI-1 rescued miR-320a-mediated biological function. BMI-1 expression was found to be up-regulated and inversely correlated with miR-320a expression in NPC. Collectively, our data indicate that miR-320a plays a tumor suppressor role in the development and progression of NPC and may be a novel therapeutic target against NPC

    Scattering of 7^{7}Be and 8^{8}B and the astrophysical S17_{17} factor

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    Measurements of scattering of 7^{7}Be at 87 MeV on a melamine (C3_{3}N6 _{6}H6_{6}) target and of 8^{8}B at 95 MeV on C were performed. For 7^{7}Be the angular range was extended over previous measurements and monitoring of the intensity of the radioactive beam was improved. The measurements allowed us to check and improve the optical model potentials used in the incoming and outgoing channels for the analysis of existing data on the proton transfer reaction 14^{14}N(7^{7}Be,8^{8}B)13^{13}C. The resultslead to an updated determination of the asymptotic normalization coefficient for the virtual decay 8^{8}B →\to 7^{7}Be + pp. We find a slightly larger value, Ctot2(8B)=0.466±0.047C_{tot}^{2}(^{8}B)=0.466\pm 0.047 fm−1^{-1}, for the melamine target. This implies an astrophysical factor, S17(0)=18.0±1.8S_{17}(0)=18.0\pm 1.8 eV⋅\cdotb, for the solar neutrino generating reaction 7^{7}Be(pp,γ\gamma )8^{8}B.Comment: 7 pages, 4 figure

    Low-mass dark matter search results from full exposure of PandaX-I experiment

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    We report the results of a weakly-interacting massive particle (WIMP) dark matter search using the full 80.1\;live-day exposure of the first stage of the PandaX experiment (PandaX-I) located in the China Jin-Ping Underground Laboratory. The PandaX-I detector has been optimized for detecting low-mass WIMPs, achieving a photon detection efficiency of 9.6\%. With a fiducial liquid xenon target mass of 54.0\,kg, no significant excess event were found above the expected background. A profile likelihood analysis confirms our earlier finding that the PandaX-I data disfavor all positive low-mass WIMP signals reported in the literature under standard assumptions. A stringent bound on the low mass WIMP is set at WIMP mass below 10\,GeV/c2^2, demonstrating that liquid xenon detectors can be competitive for low-mass WIMP searches.Comment: v3 as accepted by PRD. Minor update in the text in response to referee comments. Separating Fig. 11(a) and (b) into Fig. 11 and Fig. 12. Legend tweak in Fig. 9(b) and 9(c) as suggested by referee, as well as a missing legend for CRESST-II legend in Fig. 12 (now Fig. 13). Same version as submitted to PR
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