PPT-IceCube Calibration

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. 林貴林. IOP, NCTU. (1). F.-F. Lee and GLL, Phys. Rev. D85, 023529 (2012). (2). F.-F. Lee, GLL, . Sming. Tsai, Phys. Rev. D87, 025003 (2013). (3). . . F. .-F. Lee, GLL, . Sming. Tsai, . Phys. . Rev. D89, . The Radio Air Shower Test Array. Enhancing the IceCube Observatory. M. A. DuVernois. University of . Wisconsin. IceCube . Research Center. for the. RASTA & IceCube Collaborations. Geo-synchrotron extension to the IceTop component of the IceCube (deep in-ice + surface) experiment. Askaryan. Radio Array . A . new instrument for the detection of highest energy neutrinos.. Hagar Landsman, UW Madison. High energy neutrinos….Why ?. n + . p. +.  . P+. g. .  . p + . 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 . Remember to be alert: the data might answer questions you didn’t ask. Keith Jahoda. 29 March 2012. PCA Energy Calibration - status. Current (final) calibration is described in . Shaposhnikov. et al. “Advances in the RXTE PCA Calibration: Nearing the Statistical Limit” (in preparation). George J. Bendo. and the SPIRE-ICC. Basic Equations. Derivative of flux calibration curves (from empirical analysis):. Flux calibration curve (integral of above equation):. V. 0. is a zero-point voltage that is selected to match the background in dark sky. . USGS EROS. rmorfitt@usgs.gov. Work Performed by. SGT: Mike Choate, . Mark . Lubke, . Obaidul. . Haque. , . Ajit. . Sampath. , Jim . Storey. , . and . Esad. . Micijevic. SDSU: . Dennis . Helder. , and Ashish Shrestha . 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), Resent Discoveries and Results. Vladimir Papitashvili, Program Director. Antarctic Astrophysics & Geospace Sciences. NSF/Office of Polar Programs. Interagency Astronomy . and Astrophysics Advisory . Yicong Sui. Washington University in St. Louis. In collaboration with Bhupal Dev. Outline. Motivation:. PeV. bump in . IceCube. data. Astrophysical explanation:. Multi messenger method (Gamma Ray Constraint). results. Icíar. Montilla, . M. . Reyes, M. . Núñez. , J. Marco de la . R. osa, O. . Tubio. , M. . Puga. (. Instituto. de . Astrofísica. de Canarias). Ali . Basden. . (Durham University). GTCAO overview. University of Alabama. IceCube. . Bootcamp. 2016. Madison, WI. 6/12/16. IceCube Flashers - Bootcamp. 1. IceCube. 6/12/16. IceCube Flashers - Bootcamp. 2. Strings are numbered 1-86. DOMs are numbered 1-60, top to bottom (in ice). Matthew Fu. 1. , Timothy Govenor. 1. , Quentin King. 1. , . Parisa Roustazadeh. 1,2. , . Markus Boettcher. 3. 1. Bishop Watterson High School, Columbus, OH, USA. 2. Columbus State Community College, Columbus, OH, USA. 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..