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FRAM—F/(Ph)otometric Robotic Atmospheric Monitor is one of the atmospheric monitoring instruments at the Pierre Auger Observatory in Argentina. FRAM is anoptical telescope equipped with CCD cameras and photometer, and it automaticallyobserves a set of selected standard stars. Primarily, FRAM observations are used toobtain the wavelength dependence of the light extinction. FRAM telescope is alsoable to observe secondary astronomical targets, and namely the detection of opticalcounterparts of gamma-ray bursts has already proven to be successful. Finally, awide-field CCD camera of FRAM can be used for rapid monitoring of atmosphericconditions along the track of particularly interesting cosmic ray showers. The hardwaresetup of the telescope, its software system, data taking procedures, and resultsof analysis are described in this paper

FRAM—The Robotic Telescope for the Monitoring of the Wavelength Dependence of the Extinction: Description of Hardware, Data Analysis, and Results