Technology advancement of the CCD201-20 EMCCD for the WFIRST coronagraph instrument: sensor characterization and radiation damage

Abstract. The Wide Field InfraRed Survey Telescope-Astrophysics Focused Telescope Asset (WFIRST-AFTA) mission is a 2.4-m class space telescope that will be used across a swath of astrophysical research domains. JPL will provide a high-contrast imaging coronagraph instrument—one of two major astronomical instruments. In order to achieve the low noise performance required to detect planets under extremely low flux conditions, the electron multiplying charge-coupled device (EMCCD) has been baselined for both of the coronagraph’s sensors—the imaging camera and integral field spectrograph. JPL has established an EMCCD test laboratory in order to advance EMCCD maturity to technology readiness level-6. This plan incorporates full sensor characterization, including read noise, dark current, and clock-induced charge. In addition, by considering the unique challenges of the WFIRST space environment, degradation to the sensor’s charge transfer efficiency will be assessed, as a result of damage from high-energy particles such as protons, electrons, and cosmic rays. Science-grade CCD201-20 EMCCDs have been irradiated to a proton fluence that reflects the projected WFIRST orbit. Performance degradation due to radiation displacement damage is reported, which is the first such study for a CCD201-20 that replicates the WFIRST conditions. In addition, techniques intended to identify and mitigate radiation-induced electron trapping, such as trap pumping, custom clocking, and thermal cycling, are discussed.

[1]  James R. Janesick,et al.  Photon Transfer DN → λ , 2007 .

[2]  David Hall,et al.  Modelling charge transfer in a radiation damaged charge coupled device for Euclid , 2012, Other Conferences.

[3]  Ian S. McLean,et al.  Electronic imaging in astronomy , 2008 .

[4]  Benoit Epinat,et al.  Development of a 4k×4k frame transfer electron multiplying CCD for scientific applications , 2014, Astronomical Telescopes and Instrumentation.

[5]  David Hall,et al.  The relationship between pumped traps and signal loss in buried channel CCDs , 2013, Optics & Photonics - Optical Engineering + Applications.

[6]  David Hall,et al.  Mitigating radiation-induced charge transfer inefficiency in full-frame CCD applications by 'pumping' traps , 2012, Other Conferences.

[7]  Ralph A. Gaume,et al.  The Joint Milli-Arcsecond Pathfinder Survey: Introduction and Applications , 2009 .

[8]  Markus Loose,et al.  Detector arrays for the James Webb Space Telescope near-infrared spectrograph , 2004, SPIE Optical Engineering + Applications.

[9]  David Hall,et al.  Studying defects in the silicon lattice using CCDs , 2014 .

[10]  Andrew D. Holland,et al.  Single event gate rupture in EMCCD technology , 2012 .

[11]  René Doyon,et al.  EMCCDs: 10 MHz and beyond , 2013, Astronomical Telescopes and Instrumentation.

[12]  Cambridge,et al.  Electrode level Monte Carlo model of radiation damage effects on astronomical CCDs , 2011, 1103.3630.

[13]  R. Ingley,et al.  Proton irradiation of EMCCDs , 2006, IEEE Transactions on Electron Devices.

[14]  Olivier Daigle,et al.  CCCP: a CCD controller for counting photons , 2008, Astronomical Telescopes + Instrumentation.

[15]  Aaas News,et al.  Book Reviews , 1893, Buffalo Medical and Surgical Journal.

[16]  B. Hadwen,et al.  The noise performance of electron multiplying charge-coupled devices , 2003 .

[17]  Andrew Holland,et al.  In situ trap parameter studies in CCDs for space applications , 2014, Astronomical Telescopes and Instrumentation.

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

[19]  David Hall,et al.  An improved model of charge transfer inefficiency and correction algorithm for the Hubble Space Telescope , 2014, 1401.1151.

[20]  Edward J. Wollack,et al.  Wide-Field InfraRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA Final Report , 2013, 1305.5422.

[21]  M. Cropper,et al.  Assessment of space proton radiation-induced charge transfer inefficiency in the CCD204 for the Euclid space observatory , 2012 .

[22]  Victor A.J. Van Lint,et al.  The physics of radiation damage in particle detectors , 1987 .

[23]  D. O’Donoghue.  High speed CCD photometry , 1995 .

[24]  James W. Beletic,et al.  H2RG focal plane array and camera performance update , 2012, Other Conferences.

[25]  D. Walton,et al.  Charge-coupled devices for the ESA Euclid M-class Mission , 2012, Other Conferences.

[26]  J. Gow,et al.  Studying charge-trapping defects within the silicon lattice of a p-channel CCD using a single-trap ``pumping'' technique , 2014 .

[27]  Andrew D. Holland,et al.  Multi-level parallel clocking of CCDs for: improving charge transfer efficiency, clearing persistence, clocked anti-blooming, and generating low-noise backgrounds for pumping , 2013, Optics & Photonics - Optical Engineering + Applications.

[28]  P ? ? ? ? ? ? ? % ? ? ? ? , 1991 .

[29]  Ralf Kohley,et al.  Gaia's FPA: sampling the sky in silicon , 2012, Other Conferences.

[30]  J. Ziegler,et al.  SRIM – The stopping and range of ions in matter (2010) , 2010 .

[31]  Stephen S. Eikenberry,et al.  A Wide-Field Infrared Camera for the Palomar 200-inch Telescope , 2003, SPIE Astronomical Telescopes + Instrumentation.

[32]  R. J. Stover,et al.  A HIGH-SPEED CCD PHOTOMETER. , 1987 .

[33]  Randy Kimble.  In-flight Performance of the Detectors on HST/Wide Field Camera 3 , 2009 .

[35]  Edward A. Burke,et al.  Energy Dependence of Proton-Induced Displacement Damage in Silicon , 1986, IEEE Transactions on Nuclear Science.

[36]  M. Schmid,et al.  Investigations on performance of Electron Multiplied CCD detectors (EMCCDs) after radiation for observation of low light star-like objects in scientific space missions , 2013, Remote Sensing.

[37]  G. G. Stokes.  "J." , 1890, The New Yale Book of Quotations.

[38]  Markus Loose,et al.  Teledyne Imaging Sensors: infrared imaging technologies for astronomy and civil space , 2008, Astronomical Telescopes + Instrumentation.

[39]  Andrew D. Holland,et al.  Determination of In Situ Trap Properties in CCDs Using a “Single-Trap Pumping” Technique , 2014, IEEE Transactions on Nuclear Science.

[40]  Brian Kern,et al.  Prototype imaging spectrograph for coronagraphic exoplanet studies (PISCES) for WFIRST/AFTA , 2015, SPIE Optical Engineering + Applications.

[41]  S. T. Hodgkin,et al.  Discovery of five very low mass close binaries, resolved in the visible with lucky imaging * , 2006 .

[42]  Derek Ives,et al.  ULTRASPEC: an electron multiplication CCD camera for very low light level high speed astronomical spectrometry , 2008, Astronomical Telescopes + Instrumentation.

[43]  A. Hussain,et al.  Improving radiation tolerance in e2v CCD sensors , 2009, Optical Engineering + Applications.

[44]  W. Maes,et al.  Impact ionization in silicon: A review and update , 1990 .

[45]  James W. Beletic,et al.  4K×4K format 10μm pixel pitch H4RG-10 hybrid CMOS silicon visible focal plane array for space astronomy , 2012, Other Conferences.

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

[47]  Andrew Holland,et al.  Modelling radiation damage to ESA's Gaia satellite CCDs , 2008, Astronomical Telescopes + Instrumentation.

[48]  Benjamin Dryer,et al.  RVS Radiation Campaign 4 data II - Data Calibration , 2014 .

[49]  W. Read,et al.  Statistics of the Recombinations of Holes and Electrons , 1952 .

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

[51]  J. R. Srour,et al.  Review of displacement damage effects in silicon devices , 2003 .