99 research outputs found

    Consenso intersocietario para el tratamiento de la obesidad en adultos en Argentina

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    La obesidad es una enfermedad crĂłnica que genera altos costos en salud, cuyo tratamiento, en ocasiones, no se aborda o se lo hace de forma inadecuada, y muchas veces no se basa en la evidencia disponible. Es por ello que, a partir de una iniciativa de la Sociedad Argentina de NutriciĂłn, diferentes sociedades cientĂ­ficas se reunieron con el objetivo de construir un documento actualizado, basado en una metodologĂ­a cientĂ­fica, que aporte al mejor tratamiento de las personas que viven con obesidad en Argentina. Este es el primer Consenso Intersocietario para el tratamiento de la Obesidad en adultos en Argentina a partir del cual se obtuvieron recomendaciones para la prĂĄctica clĂ­nica basadas en la evidencia cientĂ­fica. Es una necesidad primordial contar con herramientas, adecuadas a la realidad local y consensuadas por expertos de distintas disciplinas

    Calibration of the CMS Drift Tube Chambers and Measurement of the Drift Velocity with Cosmic Rays

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    Peer reviewe

    Aligning the CMS Muon Chambers with the Muon Alignment System during an Extended Cosmic Ray Run

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    Peer reviewe

    Precise mapping of the magnetic field in the CMS barrel yoke using cosmic rays

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    This is the Pre-print version of the Article. The official published version can be accessed from the link below - Copyright @ 2010 IOPThe CMS detector is designed around a large 4 T superconducting solenoid, enclosed in a 12 000-tonne steel return yoke. A detailed map of the magnetic field is required for the accurate simulation and reconstruction of physics events in the CMS detector, not only in the inner tracking region inside the solenoid but also in the large and complex structure of the steel yoke, which is instrumented with muon chambers. Using a large sample of cosmic muon events collected by CMS in 2008, the field in the steel of the barrel yoke has been determined with a precision of 3 to 8% depending on the location.This work is supported by FMSR (Austria); FNRS and FWO (Belgium); CNPq, CAPES, FAPERJ, and FAPESP (Brazil); MES (Bulgaria); CERN; CAS, MoST, and NSFC (China); COLCIENCIAS (Colombia); MSES (Croatia); RPF (Cyprus); Academy of Sciences and NICPB (Estonia); Academy of Finland, ME, and HIP (Finland); CEA and CNRS/IN2P3 (France); BMBF, DFG, and HGF (Germany); GSRT (Greece); OTKA and NKTH (Hungary); DAE and DST (India); IPM (Iran); SFI (Ireland); INFN (Italy); NRF (Korea); LAS (Lithuania); CINVESTAV, CONACYT, SEP, and UASLP-FAI (Mexico); PAEC (Pakistan); SCSR (Poland); FCT (Portugal); JINR (Armenia, Belarus, Georgia, Ukraine, Uzbekistan); MST and MAE (Russia); MSTDS (Serbia); MICINN and CPAN (Spain); Swiss Funding Agencies (Switzerland); NSC (Taipei); TUBITAK and TAEK (Turkey); STFC (United Kingdom); DOE and NSF (USA)
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