Number of the records: 1  

New method for atmospheric calibration at the Pierre Auger Observatory using FRAM, a robotic astronomical telescope

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    SYSNO ASEP0310229
    Document TypeC - Proceedings Paper (int. conf.)
    R&D Document TypeConference Paper
    TitleNew method for atmospheric calibration at the Pierre Auger Observatory using FRAM, a robotic astronomical telescope
    TitleNové metody kalibrace atmosféry na observatoři Pierre Auger využívající robotického teleskopu FRAM
    Author(s) BenZvi, S. (US)
    Boháčová, Martina (FZU-D) RID, ORCID
    Connolly, B. (US)
    Grygar, Jiří (FZU-D) RID, ORCID
    Hrabovský, Miroslav (FZU-D) RID, ORCID
    Kárová, Tatiana (FZU-D)
    Mandát, Dušan (FZU-D) RID, ORCID
    Nečesal, Petr (FZU-D)
    Nosek, D. (CZ)
    Nožka, Libor (FZU-D) RID, ORCID
    Palatka, Miroslav (FZU-D) RID, ORCID, SAI
    Pech, Miroslav (FZU-D) RID, ORCID
    Prouza, Michael (FZU-D) RID, ORCID
    Řídký, Jan (FZU-D) RID, ORCID
    Schovánek, Petr (FZU-D) RID, ORCID
    Šmída, Radomír (FZU-D) RID
    Trávníček, Petr (FZU-D) RID, ORCID
    Vitale, P. (AR)
    Westerhoff, S. (US)
    Source TitleProceedings of the 30th International Cosmic Ray Confence. - Mexico : Universidad National Autonóma, 2007
    Pagess. 1-4
    Number of pages4 s.
    Publication formwww - www
    ActionInternational Cosmic Ray Conference /30./
    Event date03.07.2007-11.07.2007
    VEvent locationMerida
    CountryMX - Mexico
    Event typeWRD
    Languageeng - English
    CountryMX - Mexico
    KeywordsPierre Auger Observatory ; atmospheric calibration ; FRAM ; telescope
    Subject RIVBF - Elementary Particles and High Energy Physics
    R&D ProjectsLA 134 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    CEZAV0Z10100502 - FZU-D (2005-2011)
    EID SCOPUS84865771194
    AnnotationFRAM - F/(Ph)otometric Robotic Atmospheric Monitor is the latest addition to the atmospheric monitoring instruments of the Pierre Auger Observatory. An optical telescope equipped with CCD camera and photometer, it automatically observes a set of selected standard stars and a calibrated terrestrial source. Primarily, the wavelength dependence of the attenuation is derived and comparison between its vertical values and horizontal values is made. The hardware setup, software system, data taking procedures, and first analysis results are described in this paper.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2009
Number of the records: 1  

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