Abstract The next generation of neutrino telescopes will feature unprecedented sensitivities in the detection neutrinos. Here we study capabilities a large-scale telescope, like fully-operating KM3NeT experiment near future, for detecting dark matter annihilation signals from Galactic Centre. We consider both ORCA and ARCA detectors, covering masses few GeV to 100 TeV. obtain with maximum-likel...

Abstract The COMET experimental station at SEXTANTS beamline of the SOLEIL synchrotron is dedicated to coherent imaging magnetic domains, using holography and ptychography, in a sample environment including fields up 0.9 T, temperature range from 30 400 K RF pumping. 2D-detector capabilities were recently upgraded by adding standard CCD camera two new detectors: high repetition rate 2D CMOS dou...

Revised 2003 (see the various sections for authors). In this section we give various parameters for common detector components. The quoted numbers are usually based on typical devices, and should be regarded only as rough approximations for new designs. More detailed discussions of detectors and their underlying physics can be found in books by Ferbel [1], Grupen [2], Kleinknecht [3], Knoll [4]...

I give a brief introduction on gravitational wave laser interferometers, possible detectable sources from the ground and noise in the detectors. Gravitational wave research started in the early 1960's thanks to the pioneering work of Weber 1. Since that time, there has been an ongoing research effort to develop detectors of sufficient sensitivity to allow the detection of waves from astrophysic...

Vernier acuity is susceptible to degradation by image motion. The purpose of this study was to determine to what extent vernier thresholds are elevated in the presence of image motion because of reduced stimulus visibility, due to contrast smearing, or to a shift in the spatial scale of analysis. To test the visibility hypothesis, we measured vernier thresholds as a function of stimulus velocit...