Backside-illuminated, high-QE, 3e- RoN, fast 700fps, 1760x1680 pixels CMOS imager for AO with highly parallel readout

Mark Downing; Johann Kolb; Dietrich Baade; Philippe Balard; Bart Dierickx; Arnaud Defernez; Benoit Dupont; Philippe Feautrier; Gert Finger; Martin Fryer; Jean-Luc Gach; Christian Guillaume; Norbert Hubin; Olaf Iwert; Paul Jerram; Paul Jorden; Andrew Pike; Jerome Pratlong; Javier Reyes; Eric Stadler; Andrew Walker

doi:10.1117/12.925616

25 September 2012 Backside-illuminated, high-QE, 3e- RoN, fast 700fps, 1760x1680 pixels CMOS imager for AO with highly parallel readout

Mark Downing, Johann Kolb, Dietrich Baade, Philippe Balard, Bart Dierickx, Arnaud Defernez, Benoit Dupont, Philippe Feautrier, Gert Finger, Martin Fryer, Jean-Luc Gach, Christian Guillaume, Norbert Hubin, Olaf Iwert, Paul Jerram, Paul Jorden, Andrew Pike, Jerome Pratlong, Javier Reyes, Eric Stadler, Andrew Walker

Author Affiliations +

Proceedings Volume 8453, High Energy, Optical, and Infrared Detectors for Astronomy V; 84530C (2012) https://doi.org/10.1117/12.925616
Event: SPIE Astronomical Telescopes + Instrumentation, 2012, Amsterdam, Netherlands

Abstract

The success of the next generation of instruments for 8 to 40-m class telescopes will depend upon improving the image quality (correcting the distortion caused by atmospheric turbulence) by exploiting sophisticated Adaptive Optics (AO) systems. One of the critical components of the AO systems for the E-ELT has been identified as the Laser/Natural Guide Star (LGS/NGS) WaveFront Sensing (WFS) detector. The combination of large format, 1760x1680 pixels to finely sample (84x84 sub-apertures) the wavefront and the spot elongation of laser guide stars, fast frame rate of 700 (up to 1000) frames per second, low read noise (< 3e-), and high QE (> 90%) makes the development of such a device extremely challenging. Design studies by industry concluded that a thinned and backside-illuminated CMOS Imager as the most promising technology. This paper describes the multi-phased development plan that will ensure devices are available on-time for E-ELT first-light AO systems; the different CMOS pixel architectures studied; measured results of technology demonstrators that have validated the CMOS Imager approach; the design explaining the approach of massive parallelism (70,000 ADCs) needed to achieve low noise at high pixel rates of ~3 Gpixel/s ; the 88 channel LVDS data interface; the restriction that stitching (required due to the 5x6cm size) posed on the design and the solutions found to overcome these limitations. Two generations of the CMOS Imager will be built: a pioneering quarter sized device of 880x840 pixels capable of meeting first light needs of the E-ELT called NGSD (Natural Guide Star Detector); followed by the full size device, the LGSD (Laser Guide Star Detector). Funding sources: OPTICON FP6 and FP7 from European Commission and ESO.

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Mark Downing, Johann Kolb, Dietrich Baade, Philippe Balard, Bart Dierickx, Arnaud Defernez, Benoit Dupont, Philippe Feautrier, Gert Finger, Martin Fryer, Jean-Luc Gach, Christian Guillaume, Norbert Hubin, Olaf Iwert, Paul Jerram, Paul Jorden, Andrew Pike, Jerome Pratlong, Javier Reyes, Eric Stadler, and Andrew Walker "Backside-illuminated, high-QE, 3e- RoN, fast 700fps, 1760x1680 pixels CMOS imager for AO with highly parallel readout", Proc. SPIE 8453, High Energy, Optical, and Infrared Detectors for Astronomy V, 84530C (25 September 2012); https://doi.org/10.1117/12.925616

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