Showing 21–40 of 52 results
/ Date/ Name
Oct 16, 2017A gravitational-wave standard siren measurement of the Hubble constantMar 31, 2017Empirical constraints on the origin of fast radio bursts: volumetric rates and host galaxy demographics as a test of millisecond magnetar connectionJun 14, 2016A DECam Search for an Optical Counterpart to the LIGO Gravitational Wave Event GW151226May 17, 2016PS1-14bj: A Hydrogen-Poor Superluminous Supernova With a Long Rise and Slow DecayJul 21, 2015First proof of topological signature in the high pressure xenon gas TPC with electroluminescence amplification for the NEXT experimentMay 26, 2015Radon and material radiopurity assessment for the NEXT double beta decay experimentApr 14, 2015Accurate gamma and MeV-electron track reconstruction with an ultra-low diffusion Xenon/TMA TPC at 10 atmospheresNov 5, 2014Radiopurity assessment of the tracking readout for the NEXT double beta decay experimentNov 5, 2014Results of the material screening program of the NEXT experimentSep 9, 2014Ionization and scintillation of nuclear recoils in gaseous xenonNov 14, 2013Characterization of a medium size Xe/TMA TPC instrumented with microbulk Micromegas, using low-energy $γ$-raysJun 3, 2013Operation and first results of the NEXT-DEMO prototype using a silicon photomultiplier tracking arrayNov 20, 2012Initial results of NEXT-DEMO, a large-scale prototype of the NEXT-100 experimentNov 19, 2012In-situ calibration of a PMT inside a scintillation detector by means of primary scintillation detectionNov 16, 2012Radiopurity control in the NEXT-100 double beta decay experiment: procedures and initial measurementsNov 6, 2012CXOGBSJ174444.7-260330: a new long orbital period cataclysmic variable in a low stateJun 27, 2012Design and characterization of the SiPM tracking system of NEXT-DEMO, a demonstrator prototype of the NEXT-100 experimentFeb 3, 2012NEXT-100 Technical Design Report (TDR). Executive SummaryJan 10, 2012SiPMs coated with TPB : coating protocol and characterization for NEXTJul 22, 2010Calibration of the LIGO Gravitational Wave Detectors in the Fifth Science Run