Preliminary characterization results of a large format 4k × 4k EMCCD

Scientific EMCCD cameras have demonstrated excellent imaging performance under extreme low light conditions. Photon counting capability combined with a very low dark current offered by the CCD technology have made EMCCDs the detector of choice for high-performance applications such as time resolved spectroscopy and low light imaging. However, future astronomical instrumentation requires high spatial resolution while commercially available EMCCD devices are limited by a relatively modest area format of (1kx1k). To address this requirement, the Universitė de Montrėal and Teledyne-e2v have jointly developed a 4kx4k EMCCD, the CCD282. This paper presents the results of cryogenic characterization of the CCD282 operated with Nüvü Camēras’ CCD Controller for Counting Photons version 3. The advantages of a novel large format EMCCD over existing technology for high resolution spectroscopy are discussed.

[1]  N. Woolf,et al.  An optical ultrahigh-resolution cross-dispersed echelle spectrograph with adaptive optics , 2002 .

[2]  J. Hynecek Impactron-a new solid state image intensifier , 2001 .

[3]  Ray Bell,et al.  The LLCCD: low-light imaging without the need for an intensifier , 2001, IS&T/SPIE Electronic Imaging.

[4]  Sebastien Blais-Ouellette,et al.  Extreme Faint Flux Imaging with an EMCCD , 2009, 0911.4495.

[5]  David Hall,et al.  Technology advancement of the CCD201-20 EMCCD for the WFIRST coronagraph instrument: sensor characterization and radiation damage , 2015, 1601.01761.

[6]  Simon Tulloch,et al.  Secrets of E2V Technologies CCDs (ex Marconi CCDs) , 2002 .

[7]  B. Burke,et al.  Dynamic suppression of interface-state dark current in buried-channel CCDs , 1991 .

[8]  René Doyon,et al.  Astronomical imaging with EMCCDs using long exposures , 2014, Astronomical Telescopes and Instrumentation.

[9]  Olivier Daigle,et al.  The darkest EMCCD ever , 2010, Astronomical Telescopes + Instrumentation.

[10]  Bernard Delabre,et al.  Design, construction, and performance of UVES, the echelle spectrograph for the UT2 Kueyen Telescope at the ESO Paranal Observatory , 2000, Astronomical Telescopes and Instrumentation.

[11]  Erika T. Hamden,et al.  Noise and dark performance for FIREBall-2 EMCCD delta-doped CCD detector , 2015, SPIE Optical Engineering + Applications.

[12]  M. Couture,et al.  HIRES: the high-resolution echelle spectrometer on the Keck 10-m Telescope , 1994, Astronomical Telescopes and Instrumentation.

[13]  J. Janesick,et al.  Scientific Charge-Coupled Devices , 2001 .

[14]  René Doyon,et al.  Characterization results of EMCCDs for extreme low-light imaging , 2012, Other Conferences.