Showing 1–19 of 19 results
/ Date/ Name
Mar 16, 2022Deep learning applications for quality control in particle detector constructionNov 12, 2021Response of a CMS HGCAL silicon-pad electromagnetic calorimeter prototype to 20-300 GeV positronsNov 9, 2022Performance of the CMS High Granularity Calorimeter prototype to charged pion beams of 20$-$300 GeV/cNov 17, 2014Observation of the rare $B^0_s\toμ^+μ^-$ decay from the combined analysis of CMS and LHCb dataDec 10, 2020Construction and commissioning of CMS CE prototype silicon modulesDec 7, 2020The DAQ system of the 12,000 Channel CMS High Granularity Calorimeter PrototypeJun 17, 2024Using graph neural networks to reconstruct charged pion showers in the CMS High Granularity CalorimeterAug 16, 2019Modeling of rigidity dependent CORSIKA simulations for GRAPES-3Aug 30, 2000Experimental evidence for G.U.T. Proton DecayApr 19, 2013High rigidity Forbush decreases: due to CMEs or shocks?Mar 28, 2018Was the cosmic ray burst detected by the GRAPES-3 on 22 June 2015 caused by transient weakening of geomagnetic field or by an interplanetary anisotropy?May 3, 2020Energy sensitivity of the GRAPES-3 EAS array for primary cosmic ray protonsJul 21, 2000Studies of the Response of the Prototype CMS Hadron Calorimeter, Including Magnetic Field Effects, to Pion, Electron, and Muon BeamsJun 26, 2018Microscopic Characterisation of Photo Detectors from CMS Hadron CalorimeterOct 16, 2008Forbush decreases and turbulence levels at CME frontsOct 24, 2023Small-scale cosmic ray anisotropy observed by the GRAPES-3 experiment at TeV energiesMar 23, 2019Measurement of the Electrical Properties of a Thundercloud Through Muon Imaging by the GRAPES-3 ExperimentNov 12, 2019The angular resolution of GRAPES-3 EAS array after correction for the shower front curvatureApr 24, 2015How are Forbush decreases related to interplanetary magnetic field enhancements ?