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A FRAM (F/(Ph)otometric Robotic Atmospheric Monitor) telescope is a system ofa robotic mount, a large-format CCD camera and a fast telephoto lens that canbe used for atmospheric monitoring at any site when information about theatmospheric transparency is required with high spatial or temporal resolutionand where continuous use of laser-based methods for this purpose wouldinterfere with other observations. The original FRAM has been operated at thePierre Auger Observatory in Argentina for more than a decade, while three moreFRAMs are foreseen to be used by the Cherenkov Telescope Array (CTA). The CTAFRAMs are being deployed ahead of time to characterize the properties of thesites prior to the operation of the CTA telescopes; one FRAM has been runningon the planned future CTA site in Chile for a year while two others areexpected to become operational before the end of 2018. We report on thehardware and current status of operation and/or deployment of all the FRAMinstruments in question as well as on some of the preliminary results ofintegral aerosol measurements by the FRAMs in Argentina and Chile

FRAM telescopes and their measurements of aerosol content at the Pierre Auger Observatory and at future sites of the Cherenkov Telescope Array