Suzanne Ramsay is an astronomer working at the European Southern Observatory. Her interests and expertise are in optical and infrared ground based instrumentation and particularly in the development of astronomical spectrographs. Suzanne is Instrumentation Project Manager for the new 40-m class European Extremely Large Telescope, the largest optical telescope currently planned. Suzanne is an active research astronomer in the field of star formation, observing the interactions between young stars and their environments.
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This paper provides an overall summary of the AO WFS Detector requirements of the E-ELT instruments currently in design and telescope focal units. This is followed by a description of the many interesting detector, controller, and camera developments underway at ESO to meet these needs; a) the rationale behind and plan to upgrade the 240x240 pixels, 2000fps, “zero noise”, L3Vision CCD220 sensor based AONGC camera; b) status of the LGSD/NGSD High QE, 3e- RoN, fast 700fps, 1760x1680 pixels, Visible CMOS Imager and camera development; c) status of and development plans for the Selex SAPHIRA NIR eAPD and controller.
Most of the instruments and detector/camera developments are described in more detail in other papers at this conference.
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