Performance of the SLD barrel CRID during the 1992 physics data run

Performance of the SLD barrel CRID during the 1992 physics data run

Summary form only. The performance of the Cherenkov Ring Imaging Detector (CRID) of the SLD experiment at the SLAC linear collider during the 1992 physics data run is discussed. The barrel CRID is complete and fully operational. Cherenkov rings have been observed from both the liquid and the gas rad...

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Hauptverfasser: Antilogus, P., Aston, D., Bienz, T., Bird, F., Dasu, S., Dolinsky, S., Dunwoodie, W., Hallewell, G., Kawahara, H., Kwon, Y., Leith, D.W.G.S., Muller, G., Muller, D., Nagamine, T., Pavel, T.J., Ratcliff, B., Rensing, P., Schultz, D., Shapiro, S., Simopoulos, C., Solodov, E., Toge, N., Va'vra, J., Williams, S.H., Coyle, P., Coyne, D., Liu, X., Williams, D.A., Coller, J., Shank, J.T., Wilson, R.J., Whitaker, J.S., Bean, A., Caldwell, D.O., Duboscq, J., Huber, J., Lu, A., Mathys, L., McHugh, S., Witherell, M., Yellin, S., Johnson, R.A., Martinez, J., Meadows, B., Nussbaum, M., d'Oliveira, A., Santha, A.K.S., Shoup, A., Sokoloff, M.D., Stockdale, I., Baird, K., Jacques, P., Kalelkar, M., Plano, R., Stamer, P., Word, G., Abe, K., Hasegawa, K., Suekane, F., Yuta, H.
Format: Tagungsbericht
Sprache:eng
Schlagworte:
Birds
Cosmic rays
Detectors
Mirrors
Particle measurements
Particle tracking
Physics
Superluminescent diodes
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Zusammenfassung:Summary form only. The performance of the Cherenkov Ring Imaging Detector (CRID) of the SLD experiment at the SLAC linear collider during the 1992 physics data run is discussed. The barrel CRID is complete and fully operational. Cherenkov rings have been observed from both the liquid and the gas radiators. The rings are associated with particle tracks measured in the central drift chamber and the radius of the ring together with the momentum measurement is used to identify particles. Work is in progress to improve the resolution by better determining the position of the drift boxes, the mirrors, and the central drift chamber relative to one other using data from cosmic rays and Z/sup 0/ chambers.< >
DOI:10.1109/NSSMIC.1992.301120