PPT-Luminosity Calibration

Outline Motivation and Target Precision Methods 2010 Results 2011 Requests amp Strategy High b Experiments S White LHC Performance Workshop Chamonix 27 January 2011 Acknowledgments participants of the . 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 . 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. Outline:. Motivation and Target Precision. Methods . 2010 Results. 2011 Requests & Strategy. High-. b . Experiments. S. White . LHC Performance Workshop. Chamonix, 27 January 2011. Acknowledgments: participants of the . 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. Craig Markwardt & Bev . LaMarr. GSFC. PI: Keith . Gendreau. , NASA GSFC . Science: . Understanding ultra-dense matter via soft X-ray timing spectroscopy of neutron stars . Platform: International Space Station . GOES-R Program Calibration and Validation Robert A. Iacovazzi, Jr .* (1) , Edward C. Grigsby (1), Steve Goodman (2), Changyong Cao (3), Jaime Daniels (3), and Kathleen McIntyre (1) NASA (1), IceCube Calibration Overview Kurt Woschnagg University of California, Berkeley MANTS 2009 Berlin, 25 September 2009 4800 identical sensors in ultraclean, stable ice n m g geometry timing charge ice properties: 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. Oliver Brüning and . Markus . Zerlauth. HL-LHC Project Leader and Deputy Project Leader. R2E annual Meeting 2021, 2-3. rd. February 2021. Reminder of the HL-LHC Goals. 2. The main objective of HiLumi LHC Design Study is to extend the LHC lifetime by . Add 12 event classes for SVX detector. .  . Done. Generate calibration parameters for Q-vector and flattening run by run .  . on-going. Status of centrality calibration. The calibrations for run-343031-347349 are good to use..