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 . Background. Gerald L Mader. 2 . , Andria L Bilich. 1. , Charles Geoghegan. 3. 1. National Geodetic Survey, . NOAA/NOS, Boulder CO; corresponding author: . andria.bilich@noaa.gov. 1. National Geodetic Survey, NOAA/NOS, Silver Spring, MD. Republic. Helena Glaser-Opitzová, Ľudmila Ivančíková, Boris . Frankovič. European conference on quality in official statistics 2014. Vienna. 2 – 5 June 2014. Outline. calibration estimator. calibration in SO SR. Alex Fore, Simon . Yueh. , . Wenqing. Tang, Akiko Hayashi. Drift in Scatterometer Calibration. A very small drift in the scatterometer calibration can be observed over the first few months.. Magnitude of drift is order 0.1 dB. 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 . Chin-Jen Lin, George Liu. Institute of Earth Sciences, Academia . Sinica. , Taiwan. Outlines. Calibration . of the following rotational sensors. R-1 . R-2. Two applications to find . true north. Attitude . 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. Greg Holsclaw. Jan 8, 2014. 1. Outline. Calibrations since the last . meeting. Future calibrations. Calibration update. Status . of new calibration . routine. Website updates. A restructured calibration routine. 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. Radon Symposium. San Diego, California. September 21, 2016. Phillip H. Jenkins, PhD, CHP. Bowser-. Morner. , Inc.. Melinda . Ronca. -Battista. Tribal Air Monitoring Support Center, NAU. We Take it For Granted. Editor: Song . Zhi. . Checked. ：. Li . Chuanhong. Version. ：. A1001. Date. ：. 2010.10.21. The factory calibration program can be suitable for . CB448 and CB460B.. Fill 5456. LAST MEETING:. @ INJECTION:. -> Use BSRT calibration factors used before the MD. -> Compare it with WS emittances . LAST MEETING:. @ INJECTION:. -> Use BSRT calibration factors used before the MD. Presenter: Phillip S. Kott . 1. WSS. . . R . d. k. . [1 . exp. (. x. k. T. g. )]. . z. k. = . T. z . .   . 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