{"id":123,"date":"2012-03-02T15:04:21","date_gmt":"2012-03-02T15:04:21","guid":{"rendered":"http:\/\/web.auger.org.ar\/visitantes\/animus\/index.php\/2012\/03\/02\/icrc-2009-lotz-augerpapers\/"},"modified":"2012-03-02T15:04:21","modified_gmt":"2012-03-02T15:04:21","slug":"icrc-2009-lotz-augerpapers","status":"publish","type":"post","link":"https:\/\/visitantes.auger.org.ar\/index.php\/icrc-2009-lotz-augerpapers\/","title":{"rendered":"ICRC 2009 (\u0141\u00f3d\u017a) Auger Papers"},"content":{"rendered":"<ul>\n<li><a href=\"http:\/\/www.auger.org\/technical_info\/ICRC2009\/arxiv_spectrum.pdf\"><strong>The Cosmic Ray Energy Spectrum   and Related Measurements with the Pierre Auger Observatory<\/strong><\/a>,    (<a href=\"http:\/\/webhostinggeeks.com\/science\/arxiv-spectrum-ht\">Haitian-Creole translation<\/a>) including:\n<ul>\n<li>Measurement of the cosmic ray energy spectrum above 10<sup>18<\/sup> eV<\/li>\n<li>The cosmic ray flux observed at zenith angles larger than 60 degrees<\/li>\n<li>Energy calibration of data recorded with the surface detectors<\/li>\n<li>Exposure of the hybrid detector<\/li>\n<li>Energy scale derived from Fluorescence Telescopes using Cherenkov Light \t\tand Shower Universality<\/li>\n<\/ul>\n<\/li>\n<p> <\/p>\n<li><a href=\"http:\/\/www.auger.org\/technical_info\/ICRC2009\/arxiv_astrophysics.pdf\"><strong>Astrophysical Sources of Cosmic Rays   and Related Measurements with the Pierre Auger Observatory<\/strong><\/a>, including:\n<ul>\n<li>Correlation of the highest energy cosmic rays with nearby extragalactic objects<\/li>\n<li>Discriminating potential astrophysical sources of the highest energy cosmic rays<\/li>\n<li>Intrinsic anisotropy of the UHECR<\/li>\n<li>Ultra-high energy photon studies<\/li>\n<li>Limits on the flux of diffuse ultra high energy neutrinos<\/li>\n<li>Search for sidereal modulation of the arrival directions of events<\/li>\n<li>Cosmic Ray Solar Modulation Studies<\/li>\n<li>Investigation of the Displacement Angle of the Highest Energy Cosmic Rays \t\tCaused by the Galactic Magnetic Field<\/li>\n<li>Search for coincidences with astrophysical transients<\/li>\n<li>An alternative method for determining the energy of hybrid events<\/li>\n<\/ul>\n<\/li>\n<p> <\/p>\n<li><a href=\"http:\/\/www.auger.org\/technical_info\/ICRC2009\/arxiv_astrophysics.pdf\"><strong>Studies of Cosmic Ray Composition and Air Shower Structure   with the Pierre Auger Observatory<\/strong><\/a>, including:\n<ul>\n<li>Measurement of the average depth of shower maximum and its fluctuations<\/li>\n<li>Study of the nuclear mass composition of UHECR with the surface \t\tdetectors<\/li>\n<li>Comparison of data from the Pierre Auger Observatory with predictions \t\tfrom air shower simulations: testing models of hadronic interactions<\/li>\n<li>A Monte Carlo exploration of methods to determine the UHECR composition<\/li>\n<li>The delay of the start-time measured with the Pierre Auger Observatory \t\tfor inclined showers and a comparison of its variance with models<\/li>\n<li>UHE neutrino signatures in the surface detector<\/li>\n<li>The electromagnetic component of inclined air showers<\/li>\n<\/ul>\n<\/li>\n<p> <\/p>\n<li><a href=\"http:\/\/www.auger.org\/technical_info\/ICRC2009\/arxiv_calibrations.pdf\"><strong>Calibration and Monitoring of the    Pierre Auger Observatory<\/strong><\/a>, including:\n<ul>\n<li>The monitoring system of the Pierre Auger Observatory and its additional functionalities<\/li>\n<li>Atmospheric Monitoring and its Use in Air Shower Analysis<\/li>\n<li>Atmospheric effects on extensive air showers observed with the array of surface detectors<\/li>\n<li>Nightly Relative Calibration of the Fluorescence Detector<\/li>\n<li>Rapid monitoring of the atmosphere after the detection of high-energy showers<\/li>\n<li>Atmospheric Aerosol Measurements<\/li>\n<\/ul>\n<\/li>\n<p> <a href=\"http:\/\/www.auger.org\/technical_info\/ICRC2009\/arxiv_operations.pdf\"><br \/><\/a> <\/p>\n<li><a href=\"http:\/\/www.auger.org\/technical_info\/ICRC2009\/arxiv_operations.pdf\"><strong>Operations and Future Plans of the    Pierre Auger Observatory<\/strong><\/a>, including:\n<ul>\n<li>Performance and operation of the Surface Detectors<\/li>\n<li>Extension of the Pierre Auger Observatory using high-elevation fluorescence \t\ttelescopes (HEAT)<\/li>\n<li>AMIGA &#8211; Auger Muons and Infill for the Ground Array<\/li>\n<li>Radio detection of Cosmic Rays<\/li>\n<li>Hardware Developments for the AMIGA enhancement<\/li>\n<li>A simulation of the fluorescence detectors of the Pierre Auger Observatory \t\tusing GEANT 4<\/li>\n<li>Education and Public Outreach<\/li>\n<li>BATATA: A device to characterize the punch-through observed in underground  \t\tmuon detectors and to operate as a prototype for AMIGA<\/li>\n<li>Progress with the Northern Part of the Pierre Auger Observatory<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>The Cosmic Ray Energy Spectrum and Related Measurements with the Pierre Auger Observatory, (Haitian-Creole translation) including: Measurement of the cosmic ray energy spectrum above 1018 eV The cosmic ray flux observed at zenith angles larger than 60 degrees Energy calibration of data recorded with the surface detectors Exposure of the hybrid detector Energy scale derived [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_jetpack_memberships_contains_paid_content":false,"footnotes":""},"categories":[14],"tags":[],"class_list":["post-123","post","type-post","status-publish","format-standard","hentry","category-icrc-auger-papers"],"jetpack_featured_media_url":"","jetpack_sharing_enabled":true,"rttpg_featured_image_url":null,"rttpg_author":{"display_name":"PierreUser","author_link":"https:\/\/visitantes.auger.org.ar\/index.php\/author\/pierreuser\/"},"rttpg_comment":0,"rttpg_category":"<a href=\"https:\/\/visitantes.auger.org.ar\/index.php\/category\/auger\/icrc-auger-papers\/\" rel=\"category tag\">ICRC Auger Papers<\/a>","rttpg_excerpt":"The Cosmic Ray Energy Spectrum and Related Measurements with the Pierre Auger Observatory, (Haitian-Creole translation) including: Measurement of the cosmic ray energy spectrum above 1018 eV The cosmic ray flux observed at zenith angles larger than 60 degrees Energy calibration of data recorded with the surface detectors Exposure of the hybrid detector Energy scale derived&hellip;","_links":{"self":[{"href":"https:\/\/visitantes.auger.org.ar\/index.php\/wp-json\/wp\/v2\/posts\/123","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/visitantes.auger.org.ar\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/visitantes.auger.org.ar\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/visitantes.auger.org.ar\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/visitantes.auger.org.ar\/index.php\/wp-json\/wp\/v2\/comments?post=123"}],"version-history":[{"count":0,"href":"https:\/\/visitantes.auger.org.ar\/index.php\/wp-json\/wp\/v2\/posts\/123\/revisions"}],"wp:attachment":[{"href":"https:\/\/visitantes.auger.org.ar\/index.php\/wp-json\/wp\/v2\/media?parent=123"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/visitantes.auger.org.ar\/index.php\/wp-json\/wp\/v2\/categories?post=123"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/visitantes.auger.org.ar\/index.php\/wp-json\/wp\/v2\/tags?post=123"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}