Performance of the new high precision luminosity monitor of DELPHI

Autor: A. M. Zaitsev, Marco Paganoni, P. Ferrari, P.P. Trapani, Tiziano Camporesi, S. J. Alvsvaag, L. Petrovykh, Marco Bozzo, M. Espirito Santo, Ole Røhne, M. Pimenta, V. Cassio, Francesco Navarria, Ernesto Migliore, I. Kronkvist, V. Sen'ko, H. Carling, Alessandra Romero, A. Klovning, G. Della Ricca, B. Tome, L. Lanceri, G.P. Barreira, A. Onofre, M. Bigi, I. Gouz, R. Cereseto, R. Mazza, F. Chignoli, A. N. Karyukhin, I. Ivanyushenkov, Vincent Hedberg, M. Guerzoni, Evgueni Vlasov, F. Terranova, L. Simonetti, Roberto Leoni, M. Prest, Andrea Perrotta, A. Maio, D.R. Dharmasiri, M. Bari, V. Giordano, Alberto Benvenuti, M. Pegoraro, E. Vallazza, P. Negri, B. Nossum, A. Konopliannikov, L. Castellani, A. B. Fenyuk, P. Poropat, V. Obraztsov, N. Shalanda, M. Bonesini, D. Gamba, O.A. Maeland, Bernhard Skaali, S. Gumenyuk, Alexander Lincoln Read, Goeran Jarlskog, E. Falk, Luis Peralta
Přispěvatelé: DELLA RICCA, Giuseppe, Lanceri, Livio, Poropat, Paolo
Jazyk: angličtina
Rok vydání: 1997
Předmět:
Zdroj: CIÊNCIAVITAE
Scopus-Elsevier
Popis: The STIC calorimeter was installed in the DELPHI detector in 1994. The main goal is to measure the luminosity with an accuracy better than 0.1%. The calorimeter was built using the “Shashlik” technique. The light is collected by wavelength shifting fibers and readout by phototetrodes that can operate inside the magnetic field. The detector performance during the 1994–1995 data taking is presented. The different contributions to the systematic error on the luminosity measurement are discussed.
Databáze: OpenAIRE