Comments from Anna. Comment 1. Triggers : as discussed during meeting – consider move to higher offline lepton pT cut or check data/MC agreement for slope of the turn on curve of used triggersBy baruch
WG7 summary and Science Plan. Chiara Marsigli ARPA Emilia-Romagna, SIMC. COSMO-E setup. Ensemble forecasts with convection-permitting resolution (2.2 km mesh-size) 21 members T wice a day up to +120h for Alpine area (15% larger than COSMO-2 domain)By napua
Introduction. Ricardo Goncalo HSG5 H->bb weekly meeting, 25 October 2011. News! News! News!. Peak stable lumi stable 3.59x10 33 cm -2 s -1 5.09 fb -1 with stable beams collected so far – 21 pb -1 collected last week 5.45 fb -1 deliveredBy bendek
Search for the QCD Critical Point. Gary D. Westfall Michigan State University For the STAR Collaboration. Search for Possible QCD Critical Point. Trajectories at low μ B Theories suggest a cross-over transition. Trajectories at high μ B Theories suggest a first-order transition.By flynn
Suppression of the low-energy noise: an improved approach. EPIC-pn detector noise. 50.7 ks closed FF (rev 059). Quadrant 0. adu. Suppression of the EPIC-pn detector noise. Original method (“method 1”), implemented in the SAS task epreject :By cicero
Heavy Flavor Production at the Tevatron. Jennifer Pursley The Johns Hopkins University on behalf of the CDF and D0 Collaborations. Beauty 2006 - University of Oxford, UK September 25-29, 2006. Focus of this talk. BRAND NEW RESULT! S b (*)± searchBy ronna
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