193 research outputs found

    Study of the flying ability of Rhynchophorus ferrugineus (Coleoptera: Dryophthoridae) adults using a computer-monitored flight mill

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    The red palm weevil, Rhynchophorus ferrugineus (Olivier) (Coleoptera: Dryophthoridae), native to tropical Asian regions, has become a serious threat to palm trees all over the world. Knowledge of its flight potential is vital to improving the preventive and curative measures currently used to manage this pest. As R. ferrugineus is a quarantine pest, it is difficult to study its flight potential in the field. A computer-monitored flight mill was adapted to analyse the flying ability of R. ferrugineus through the study of different flight parameters (number of flights, total distance flown, longest single flight, flight duration, and average and maximum speed) and the influence of the weevil s sex, age, and body size on these flight parameters. Despite significant differences in the adult body size (body weight and length) of males and females, the sex of R. ferrugineus adults did not have an influence on their flight potential. Neither adult body size nor age was found to affect the weevil s flying abilities, although there was a significantly higher percentage of individuals flying that were 8 23 days old than 1 7 days old. Compared to the longest single flight, 54% of the insects were classified as short-distance flyers (covering <100m) and 36 and 10% were classified as medium- (100 5000m) and long-distance (> 5000m), respectively. The results are compared with similar studies on different insect species under laboratory and field conditions.The authors wish to thank researcher Daniel Sauvard (INRA - Unite de Zoologie Forestiere - Orleans) for helping in the knowledge of the flight mill technique. For the help in the design and construction of the flight mill device, we thank Anna Comes and Inaki Moratal. For the reviews on the previous versions of this manuscript, we thank Ferran Garcia-Mari (Universitat Politecnica de Valencia - Instituto Agroforestal del Mediterraneo) and Apostolos Pekas (Biobest Belgium N. V.). This research was partially funded by the Foundation of the Comunidad Valencia for the Agroalimentary Research, Agroalimed, within the project named: Study of the flight behaviour and chromatic attraction in Rhynchophorus ferrugineus adults (Coleoptera: Curculionidae).Ávalos Masó, JA.; Martí Campoy, A.; Soto Tornero, MT. (2014). Study of the flying ability of Rhynchophorus ferrugineus (Coleoptera: Dryophthoridae) adults using a computer-monitored flight mill. Bulletin of Entomological Research. 104(4):462-467. doi:10.1017/S0007485314000121S4624671044OEPP/EPPO (2008). Rhynchophorus ferrugineus. Data sheets on quarantine pests. Available online at http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2338.2008.01195.x/pdf.Heath, R. R., Coffelt, J. A., Sonnet, P. E., Proshold, F. 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    Phase I and pharmacokinetic study of the polyamine synthesis inhibitor SAM486A in combination with 5-fluorouracil/leucovorin in metastatic colorectal cancer

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    PURPOSE: The purpose of our study was to determine the maximum-tolerated\n dose, dose-limiting toxicity, safety profile, and pharmacokinetics of the\n polyamine synthesis inhibitor SAM486A given in combination with\n 5-fluorouracil/leucovorin (5-FU/LV) in cancer patients. EXPERIMENTAL\n DESIGN: Patients with advanced colorectal cancer were treated with 5-FU\n [bolus (400 mg/m(2)) followed by a 22-h infusion (600 mg/m(2))] and LV\n (200 mg/m(2)) and escalating doses of SAM486A, 1-3-h infusion daily for 3\n days. Plasma sampling was performed to characterize the pharmacokinetics\n and pharmacodynamics of the combination RESULTS: Twenty-seven patients\n with metastatic colorectal cancer and 1 with pseudomyxoma peritonei were\n treated. Twenty-six patients received SAM486A in the combination at doses\n ranging from 25 to 150 mg/m(2)/day. Dose-limiting toxicity consisting of\n fatigue grade 3 was seen at 150 mg/m(2)/day. Other adverse events included\n neutropenia, hand and foot syndrome, nausea, vomiting, diarrhea, and\n constipation. Fifteen of 26 patients evaluable for best response according\n to the Southwest Oncology Group criteria achieved a partial response [8\n (30%) of 26] or stable disease [9 (35%) of 26]. SAM486A did not influence\n the pharmacokinetics of 5-FU, and SAM486A clearance was similar to that\n when used as a single agent. CONCLUSIONS: The novel molecular agent\n SAM486A is tolerable and safe in combination with a standard 5-FU regimen\n in patients with advanced colorectal cancer. The dose of SAM486A\n recommended for additional studies with this combination is 125\n mg/m(2)/day. A disease-directed evaluation of SAM486A using this regimen\n is warranted

    Design of adjustable Tuned Mass Dampers using elastomeric O-rings

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    Tuned mass dampers (TMDs) are widely used in passive vibration control, and have been implemented on many engineering structures. In general, the design of TMDs is unique to each application; the choice of damping material and its in-situ performance are key issues that can affect design and prototyping costs. The present contribution demonstrates that TMDs can be built using ubiquitous and low-cost elastomeric O-rings. It is shown that the damping and stiffness characteristics of the O-ring can be predicted a priori, in order to achieve an initial design that is fit for purpose. Furthermore, it is shown that the nonlinear characteristics of the O-ring enable the device to be easily tuned in-situ, in order to optimise the final system. Finally, the simple configuration of the device makes it well suited to through-mounting or surface-mounting on thin-walled flexible structures such as beams and plates

    Quality control for the first large areas of triple-GEM chambers for the CMS endcaps

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    The CMS Collaboration plans to equip the very forward muon system with triple-GEM detectors that can withstand the environment of the High-Luminosity LHC.This project is at the final stages of R&D and moving to production. A large area of several 100 m 2 are to be instrumented with GEM detectors which will be produced in six different sites around the world. A common construction and quality control procedure is required to ensure the performance of each detector.The quality control steps will include optical inspection,cleaning and baking of all materials and parts used to build the detector,leakage current tests of the GEM foils,high voltage tests,gas leak tests of the chambers and monitoring pressures time,gain calibration to know the optimal operation region of the detector,gain uniformity tests, and studying the efficiency,noise and tracking performance of the detectors in a cosmic stand using scintillator

    Measurement of Atmospheric Neutrino Oscillations with the ANTARES Neutrino Telescope

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    The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximum mixing, a mass difference of Δm322=(3.1±0.9)103\Delta m_{32}^2=(3.1\pm 0.9)\cdot 10^{-3} eV2^2 is obtained, in good agreement with the world average value.Comment: 9 pages, 5 figure

    The ANTARES Optical Beacon System

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    ANTARES is a neutrino telescope being deployed in the Mediterranean Sea. It consists of a three dimensional array of photomultiplier tubes that can detect the Cherenkov light induced by charged particles produced in the interactions of neutrinos with the surrounding medium. High angular resolution can be achieved, in particular when a muon is produced, provided that the Cherenkov photons are detected with sufficient timing precision. Considerations of the intrinsic time uncertainties stemming from the transit time spread in the photomultiplier tubes and the mechanism of transmission of light in sea water lead to the conclusion that a relative time accuracy of the order of 0.5 ns is desirable. Accordingly, different time calibration systems have been developed for the ANTARES telescope. In this article, a system based on Optical Beacons, a set of external and well-controlled pulsed light sources located throughout the detector, is described. This calibration system takes into account the optical properties of sea water, which is used as the detection volume of the ANTARES telescope. The design, tests, construction and first results of the two types of beacons, LED and laser-based, are presented.Comment: 21 pages, 18 figures, submitted to Nucl. Instr. and Meth. Phys. Res.

    Anisotropy studies around the galactic centre at EeV energies with the Auger Observatory

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    Data from the Pierre Auger Observatory are analyzed to search for anisotropies near the direction of the Galactic Centre at EeV energies. The exposure of the surface array in this part of the sky is already significantly larger than that of the fore-runner experiments. Our results do not support previous findings of localized excesses in the AGASA and SUGAR data. We set an upper bound on a point-like flux of cosmic rays arriving from the Galactic Centre which excludes several scenarios predicting sources of EeV neutrons from Sagittarius AA. Also the events detected simultaneously by the surface and fluorescence detectors (the `hybrid' data set), which have better pointing accuracy but are less numerous than those of the surface array alone, do not show any significant localized excess from this direction.Comment: Matches published versio

    Departure from the vogel behaviour in the glass transition region-thermally stimulated recovery, creep and dynamic mechanical analysis studies

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    In this work the study of the dynamics of the segmental motions close to Tg of a poly(methyl methacrylate), PMMA, network was analysed by distinct mechanical spectroscopy techniques. Three techniques were employed: dynamic mechanical analysis (DMA), creep and thermally stimulated recovery (TSR). The time–temperature superposition principle was applied to the DMA and creep results, and master curves were successfully constructed. A change from a Vogel to an Arrhenius behaviour was observed in these results. Above Tg it was found a distinct temperature dependence for the retardation times calculated from creep and the relaxation times calculated from DMA. This unexpected behaviour was attributed to the merging of the a and the b relaxations that occurs in PMMA systems. The apparent activation energies ðEaÞ were also calculated from DMA, creep and TSR experiments. Above Tg the Ea values obtained agreed very well for all the techniques. In addition, the fragility exhibited by this material was investigated by the mechanical spectroscopy techniques referred above and by differential scanning calorimetry (DSC). The obtained values of the fragility index m indicated that the PMMA network is a kinetically fragile system. The thermodynamic manifestation of the fragility was also analysed

    A First Search for coincident Gravitational Waves and High Energy Neutrinos using LIGO, Virgo and ANTARES data from 2007

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    We present the results of the first search for gravitational wave bursts associated with high energy neutrinos. Together, these messengers could reveal new, hidden sources that are not observed by conventional photon astronomy, particularly at high energy. Our search uses neutrinos detected by the underwater neutrino telescope ANTARES in its 5 line configuration during the period January - September 2007, which coincided with the fifth and first science runs of LIGO and Virgo, respectively. The LIGO-Virgo data were analysed for candidate gravitational-wave signals coincident in time and direction with the neutrino events. No significant coincident events were observed. We place limits on the density of joint high energy neutrino - gravitational wave emission events in the local universe, and compare them with densities of merger and core-collapse events.Comment: 19 pages, 8 figures, science summary page at http://www.ligo.org/science/Publication-S5LV_ANTARES/index.php. Public access area to figures, tables at https://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=p120000
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