PPT-Collimation and Star Testing

Author : pasty-toler | Published Date : 2017-09-29

An RVAS Meeting Program By Frank Baratta March 20 2017 Horsehead Nebula Public domain image at PixaBaycom F Baratta 2017 Graphics and images F Baratta 2017 except

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Collimation and Star Testing: Transcript


An RVAS Meeting Program By Frank Baratta March 20 2017 Horsehead Nebula Public domain image at PixaBaycom F Baratta 2017 Graphics and images F Baratta 2017 except as noted bad collimation is the number one killer of telescopes world wide . By observing outoffocus star images you can test whether your telescopes optics are aligned Place a star in the centre of the field of view and move the focuser so that the image is slightly out of focus If the seeing conditions are good you will se Alessandro . variola. , . lal. - in2p3 – . cnrs. Thanks. to . T.Demma. , . L.Burmistov. UA9 is the crystal-assisted collimation experiment at CERN. . The aim of this experiment is to demonstrate that bent crystals can work as a “smart deflector” on primary halo particles. Bruce C. Brown. Main Injector Department. 29 July 2015. Meeting Outline. BCBrown.            (5 min) Introduction and Issues . Igor . Tropin.          (15 min)     Status MARS/MAD-X Tools. R. Assmann. 25.3.2010. Joint Meeting SPS Upgrade Study Group and SPS Task Force. Introduction. This is a brain-storming talk.. No detailed technical work done but enough to . explore and discuss a collimation option for SPS. Bien . positionner le miroir secondaire devant le . porte-oculaire. Normalement, ceci n'aurait pas à être fait plus d'une fois, soit la première fois que vous utilisez un nouveau télescope. Par le petit trou de l’oculaire de collimation vous devriez voir le miroir secondaire avec le miroir primaire qui s'y réfléchit. Le miroir secondaire devrait paraître centré et bien rond. . reach. R. . . Bruce, . R. Assmann,. M. . Cauchi. , D. . Deboy. , L. . Lari, . S. . . Redaelli, A. . Rossi, . B. . Salvachua, G. . Valentino. Acknowledgements. :. W. . Herr, . M. Lamont, R. . de . Maria, . Zhirong . Huang. March 6, 2012. FLS2012 Workshop, Jefferson Lab. Outline. Introduction. Seeding and TW. Attosecond. pulses. Better beams. SASE wavelength range: . 25 – 1.2 . Å. Photon energy range: . Tully . Baetz. Raymond Dao. Caleb . Ogg. 1. Mission Statement. The . DemoSat. . Project shall test several components of . the ALL-STAR mission in order to reduce risks in those areas. . Mission Objectives. Skordis. . & F. . Cerutti. loss input by: E. . Quaranta. , R. Bruce and S. . Redaelli. Protection screen design with: . P. Fessia , L. . Favre. ,. . P. A. . Thonet. 2/9/2013 Collimation Working Group. France I. Rousselle, J. Farah, F. Dufay, A. Noel1,3, C. Corbet, N. Rossetto, C. Mabit, B. Royer, L. Gonzalez Keywords: Action 9 - Facilitation of research in advanced topics of radiation protectio beam in UA9. W. Scandale. Historical perspective. RD22 at the CERN-SPS as a test bed of beam extraction at LHC. E853 at the FNAL-. Tevatron. as a test bed for the SSC. T. he CERN-INTAS programmes on crystal technology. TeV. R. Bruce, . A. Mereghetti. , S. Redaelli, B. . Salvachua. rMPP. . Meeting, CERN, . 26. th. Oct . 2015. DS . downstream of . IR7. :. Affected by . leakage. from . betatron. . collimation. system (single diffractive events);. Self-Testing: Evidence for Action: Key Findings from the HIV . S. elf-. T. esting . A. f. r. ica (STAR) Project in Malawi, Zambia and . Zimbabwe . Prof. Anne-Claude Crémieux. Hôpital Saint-Louis. Université Paris 7. Assessment Department. Dr. Bertha Doar. Director of Assessment. Assessment Office. 2014. Introductions . - Assessment . Department. Duties and functions. Changes to Assessment for FY15. None of the assessments predict state test performance for FY15.

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