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FRAM - the robotic telescope for the monitoring of the wavelength dependence of the extinction: description of hardware, data analysis, and results

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    SYSNO ASEP0355338
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JOstatní články
    TitleFRAM - the robotic telescope for the monitoring of the wavelength dependence of the extinction: description of hardware, data analysis, and results
    Author(s) Prouza, Michael (FZU-D) RID, ORCID
    Jelínek, M. (ES)
    Kubánek, P. (ES)
    Ebr, Jan (FZU-D) RID, ORCID
    Trávníček, Petr (FZU-D) RID, ORCID
    Šmída, Radomír (FZU-D) RID
    Number of authors6
    Source TitleAdvances in Astronomy - ISSN 1687-7969
    Roč. 2010, - (2010), 849382/1-849382/5
    Number of pages5 s.
    Languageeng - English
    CountryUS - United States
    KeywordsFRAM ; wavelength dependence ; light extinction ; cosmic ray showers
    Subject RIVBF - Elementary Particles and High Energy Physics
    R&D ProjectsLC527 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    LA08016 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    CEZAV0Z10100502 - FZU-D (2005-2011)
    AV0Z10100523 - FZU-D (2005-2011)
    DOI10.1155/2010/849382
    AnnotationFRAM - F/(Ph)otometric Robotic Atmospheric Monitor is one of the atmospheric monitoring instruments at the Pierre Auger Observatory in Argentina. FRAM is an optical telescope equipped with CCD cameras and photometer, and it automatically observes a set of selected standard stars. Primarily, FRAM observations are used to obtain the wavelength dependence of the light extinction. FRAM telescope is also able to observe secondary astronomical targets, and namely the detection of optical counterparts of gamma-ray bursts has already proven to be successful. Finally, a wide-field CCD camera of FRAM can be used for rapid monitoring of atmospheric conditions along the track of particularly interesting cosmic ray showers. The hardware setup of the telescope, its software system, data taking procedures, and results of analysis are described in this paper.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2011
Number of the records: 1  

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