Greisen-Zatsepin-Kuzmin (GZK): Cosmic ray protons 1019.5 eV will be ... ANITA sees 'skimmers'. The ANITA Collaboration. University of California at Irvine ...
Greisen-Zatsepin-Kuzmin(GZK) Limit. Cosmic rays with energies above 5 1019 eV will interact with the cosmic ... This process would continue until the energy of ...
No clue of GZK cut @ 5 1019 ? JPM- LAPP-Les Houches ... The GKZ cut-off ... interest because of the 'GZK cut-off' (Greisen, 1966; Zatsepin and Kuz'min, 1966) ...
... released today for DC2 analyses; Jean Ballet and David Landriu are producing it ... for 25 years in astronomy; Wells, Greisen, & Harten (1981, A&AS, 44, 363) ...
... AGASA spectrum 100 events/yr above 1020 eV * View of Los Leones Fluorescence Site * The Fluorescence Detector 3.4 m spherical mirror PMT camera Spherical ...
Cascadas Electromagn ticas. Por Mariana. Para el seminario Introducci n a la ... M todos Monte Carlo expresiones exactas para las secciones eficaces ...
Risco dobrado de graves malforma es: Hansen M et al: The risk of major birth defects after intracytoplasmic sperm injection and in vitro fertilisation.
The Auger hybrid concept. Almost completely operating, now 1 year full observatory ! ... this probability needs 'penalization' i.e. Pfin = P/Nt (from MC)? z 0.018 ...
Sophia Children s Hospital Family-Centered Care: From bench to bedside and back Jos M. Latour RN, PhD Nurse Scientist * * Content Relevance of these areas to ...
anisotropy expectations. for different AGN types. Takami, SI , in prep. ... characteristic spectra, anisotropy, composition. hard X-rays TeV gamma-rays. AGNs ...
Manfred Hanke, August 2005: (guided by Prof. A. Sch fer) QED-Project Compton-scattering of the cosmic background radiation off a ultrarelativsitic cosmic proton
Space Monkeys and the Threat to Spacetime. History of Anti-Space ... SN1006 (Winkler et al. 2003) Went off in AD 1006. G.326.6 14.6. D=2.2kpc. z=555pc. R=6.8kpc ...
A Cross Check of Atmospheric Attenuation for the High Resolution Fly s Eye Astroparticle Experiment Chris Cannon Advisor: Lawrence Wiencke University of Utah
... wakefield (Acceleration Gradient G) excited by whistler wave in magnetized plasma is ... Simulations for production of whistler wave packet is also in progress. ...
Ultra High Energy Cosmic Rays. Glennys R. Farrar. Center for Cosmology ... 1927 Cosmic rays ... CHICOS (Los Angeles): low resolution, large area http://www. ...
Is the End in Sight for Ultrahigh Energy Cosmic Rays (UHECR) ... Cosmologically distance gamma-ray burst model (hep-ph/0206217) Galactic cosmic rays ...
High-energy emission from the tidal disruption of stars by massive black holes---preliminary results Xiang-Yu Wang Nanjing University, China Collaborators: K. S ...
(a) Physics Department, Nuclear and Particle Physics Section, University of ... Primary energy of a cosmic particle is proportional to the total number of ...
Distancia de la estaci n m s cercana al punto de impacto medida en el plano de la lluvia. ... en la Estaci n m s Cercana. Simulaciones de las lluvias: Aires ...
Sampling 'Hysteresis' Reference observations. Use edge pixels @ no ... 'Hysteresis' From inaccurate time tags for either telescope positions or data samples ...
... and it remains unique to solve the homogeneity and isotropy puzzle in UHECR data: ... related to UHECR : Isotropy in AGASA, HIRES and AUGER still favour cosmic ...
Skobeltsyn Institute of Nuclear Physics of MSU, Joint Institute of Nuclear Research, Dubna ... In the TUS telescope it consisted of 6 Fresnel type mirror segments. ...
... submission, and handling of ... submitted manually or chosen dynamically (think of Barry Clark for the VLA) ... Led by Sanjay Bhatnagar, Steve Myers ...
Title: Nessun titolo diapositiva Author: bruno Last modified by: Cliente Created Date: 10/2/2004 2:16:27 PM Document presentation format: Apresenta o na tela
For Sources with tgp 1: Strongest know z evolution (QSO, SFR) ... tgp for known sources. ep. e'g. n. p e e- eg. Antares (0.1 Gton) Nemo (1 Gton) Anita ...
Constraining UHECR source spectrum from observations in GZK regime ... Convolve result with experimental exposure and take into account energy resolution. ...
For SOFT processes the rates and properties are dominated by non-perturbative QCD effects ... Pierre Auger Observatory: - New arsenal of 'hybrid' data. ...
Need to multiply by cross sections and convolve along lines of sight. ... As for gamma-rays, need to convolve the electron CR spectrum with the Galactic ...
E-165 FLASH Measurement of Air Fluorescence Produced by Air Showers. UHECR Spectrum AGASA vs HiRes Fetish - style of the Atie/Atye/Attie/Attye from Ivory Coast ...
GORU E TEME U ASTROFIZICI Bojan Arbutina Katedra za astronomiju Matemati kog fakulteta Univerziteta u Beogradu arbo@math.rs nere eni problemi u astrofizici gama ...
AUGER experiment combining ground array with fluorescence such. will resolve most of this issues in 1-2 years from now. Statistics ... relict background n and g ...
Registry of FITS Conventions. WCS standards for Distortions and Time. New FITS Standard Document ... ESO HIERARCH keyword (under review) More conventions to be added ...