Repositorio Institucional de la Universidad de Oviedo

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Tim Stelzer and Fabio Maltoni have provided particularly valuable assistance in the estimation of standard model backgrounds. Sergey Alekhin provided helpful correspondence in understanding the theoretical uncertainties on W and Z production imposed as constraints on the Vista correction factor fit. Sascha Caron provided insight gained from the general search at H1. Torbjörn Sjöstrand assisted in the understanding of Pythia’s treatment of parton showering applied to the Vista 3j ΔR(j2,j3) discrepancy. We thank the Fermilab staff and the technical staffs of the participating institutions for their vital contributions. This work was supported by the U.S. Department of Energy and National Science Foundation; the Italian Istituto Nazionale di Fisica Nucleare; the Ministry of Education, Culture, Sports, Science and Technology of Japan; the Natural Sciences and Engineering Research Council of Canada; the National Science Council of the Republic of China; the Swiss National Science Foundation; the A. P. Sloan Foundation; the Bundesministerium für Bildung und Forschung, Germany; the Korean Science and Engineering Foundation and the Korean Research Foundation; the Science and Technology Facilities Council and the Royal Society, UK; the Institut National de Physique Nucleaire et Physique des Particules/CNRS; the Russian Foundation for Basic Research; the Comisión Interministerial de Ciencia y Tecnología, Spain; the European Community’s Human Potential Programme; the Slovak R&D Agency; and the Academy of Finland.