Wavelength Shifters for Water Cherenkov Detectors

The light yield of a water-based Cherenkov detector can be significantly improved by adding a wavelength shifter. Wavelength shifter (WLS) molecules absorb ultraviolet photons and re-emit them at longer wavelengths where typical photomultiplier tubes are more sensitive. In this study, several wavelength shifter compounds are tested for possible deployment in the Sudbury Neutrino Observatory (SNO). Test results on optical properties and chemical compatibility for a few WLS candidates are reported; together with timing and gain measurements. A Monte Carlo simulation of the SNO detector response is used to estimate the total light gain with WLS. Finally, a cosmic ray Cherenkov detector was built to investigate the optical properties of WLS.Comment: 13 pages, 3 figure

Nine loci for ocular axial length identified through genome-wide association studies, including shared loci with refractive error

10.1016/j.ajhg.2013.06.016American Journal of Human Genetics932264-277AJHG