Development and use of an L3CCD high-cadence imaging system for Optical Astronomy

A high cadence imaging system, based on a Low Light Level CCD (L3CCD) camera, has been developed for photometric and polarimetric applications. The camera system is an iXon DV-887 from Andor Technology, which uses a CCD97 L3CCD detector from E2V technologies. This is a back illuminated device, giving it an extended blue response, and has an active area of 512x 512 pixels. The camera system allows frame-rates ranging from 30 fps (full frame) to 425 fps (windowed binned frame). We outline the system design, concentrating on the calibration and control of the L3CCD camera. The L3CCD detector can be either triggered directly by a GPS time-server frequency generator or be internally triggered. A central PC remotely controls the camera computer system and timeserver. The data is saved as standard FITS files. The large data loads associated with high frame rates, leads to issues with gathering and storing the data effectively. To overcome such problems, a specific data management approach is used, and a Python PYRAF data reduction pipeline was written for the Linux environment. This uses calibration data collected either on-site, or from lab based measurements, and enables a fast and reliable method for reducing images. To date, the system has been used twice on the 1.5m Cassini Telescope in Loiano (Italy); we present the reduction methods and observations made.