PPT-Luminosity and time estimates

Mike Lamont Thanks for discussion R Assmann R Bailey M Ferro Luzzi S Fartoukh O Bruning The future is a strange place Aim of the exercise is to establish some realistic numbers given accepted constraints. G. Arduini – BE/ABP. Contributions by: M. C. Alabau-Pons, O.O. Andreassen, V. Chareyre, R. De Maria, G. Golluccio, W. . Höfle. , J-B Jeanneret, L. Walckiers. Effect on luminosity:. Injection. Collision. Redshifts. Gordon Richards. Drexel University. With thanks to. Michael Strauss, . Xiaohui. Fan, Don Schneider, and . Linhua. Jiang. Quasar Luminosity Function. Croom. et al. 2004. Space density of quasars as a function of . Capetti. , . R. Baldi, B. Balmaverde, S. Buttiglione. AGN 10 - Roma 10/09/2012. WHY AN AGN CENSUS?. A PROPER AGN CENSUS IS NEEDED FOR A VARIETY OF STUDIES, SUCH AS, . E.G.. , THE AGN/HOST GALAXY CONNECTION, THE PROPERTIES OF THE CENTRAL ENGINE, THE AGN LUMINOSITY FUNCTION . Frank Zimmermann. HL-LHC/LIU brainstorming . Jiva. Hill, 24 June 2011. n. o beam-beam limit . l. imit on total beam current in LHC [& SPS] . due to several systems (RF, dump, vacuum, collimator robustness, machine protection, RP, …) at ultimate value. Yue . Shen. Carnegie Observatories. In collaboration with Brandon . Kelly (UCSB). M. otivation. T. he abundance (and clustering) of quasars are key to understand the evolution of quasars/SMBHs in the hierarchical structure formation paradigm . IR optics. José L. Abelleira, PhD candidate EPFL, CERN BE-ABP. Supervised by F. Zimmermann, CERN Beams dep.. Thanks to: . O.Domínguez. . S . Russenchuck. , . D.Shatilov. , M.. . Zobov. CERN, 22. th. Timothy Costigan. Kyoungah See. 1. Outline. Motivation of Topic. Review Practice in Therapeutic Areas. Issues in Implementation . Type 1 error inflation. Transformations. Estimation of Variance. Simulation Study. 2. Overview. What are multiyear estimates?. When should you use multiyear estimates?. What should you be aware of when using multiyear estimates?. How can you use multiyear estimates to make comparisons?. Jack . Singal. University of Richmond. Stat. . Chall. . In 21. st. Century Cosmology. May 25, 2016. J. Singal, U. Richmond. V. . Petrosian. , Stanford. Orientation. What we have. :. Flux-limited survey catalogs. conditions. F. Antoniou, . M. . Hostettler, . Y. Papaphilippou. , . S.Papadopoulou. ,. . G. . Papotti. . . Acknowledgements: . Beam-Beam . and Luminosity studies working group, G. . Arduini. , G. . Bunch currentBeam energyRepetition frequency Number of bunches 4 per beamHorizontal emittanceVertical emittanceMax luminosity2 BEAM DIAGNOSTICSThe BEUV telescopes detect the synchrotron light emit-te Bunch currentBeam energyRepetition frequency Number of bunches 4 per beamHorizontal emittanceVertical emittanceMax luminosity2 BEAM DIAGNOSTICSThe BEUV telescopes detect the synchrotron light emit-te Samir . Arfaoui. Stony Brook University. 5 December 2011. Samir Arfaoui - LAr Week. 1. Measurement principle. 7 December 2011. Samir Arfaoui - LAr Week. 2. Pros:. Trigger independent. DAQ independent. . FERRO-LUZZI , LHC . Programme. Coordinator. CERN - PH Dept.. Overview of machine progress. rough chronology, recent achievement, current status. Luminosity calibration. s. 1/2. = 0.9 & 7 TeV.