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Noiseless, high frame rate (> kHz), photon counting arrays for use in the optical to extreme UV
John Vallerga, Jason McPhate, Anton Tremsin and Oswald Siegmund Space Sciences Laboratory, University of California, Berkeley Bettina Mikulec and Allan Clark University of Geneva
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Future WFS detector requirements
High optical QE for fainter guide stars Lots of pixels - eventually 512 x 512 More accuators More complex LGS images (parallax, gated, etc) Off null / open loop operation Very low (or zero!) readout noise kHz frame rates
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Photon Counting Charge integrating Events Q V ± sv Events ± sEvents
Threshold Events Count (x,y,t) Charge integrating Q ADC V ± sv Events ± sEvents
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Centroid in presence of noise:
8 x 8 Noiseless 35% QE 10 photons - 100 photons 1000 photons 8 x e- rms 90% QE 6 x e- rms 90% QE 4 x e- rms 90% QE
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Centroid error vs. input fluence
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Imaging, Photon Counting Detectors
Photocathode converts photon to electron MCP(s) amplify electron by 104 to 108 Rear field accelerates electrons to anode Patterned anode measures charge centroid
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Bandpass by photocathode selection
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MCP Detectors at SSL Berkeley
COS FUV for Hubble (200 x 10 mm windowless) 25 mm Optical Tube GALEX 68 mm NUV Tube (in orbit)
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Wavefront Sensor Event Rates
5000 centroids Kilohertz feedback rates (atmospheric timescale) 1000 detected events per spot for sub-pixel centroiding 5000 x 1000 x 1000 = 5 Gigahertz counting rate! Requires integrating detector
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Our AO detector concept
An optical imaging tube using: GaAs photocathode MCPs to amplify to ~104 Medipix2 ASIC readout
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Medipix2 ASIC Readout Each pixel has amp, discriminator, gate & counter. 256 x 256 with 55 µm pixels (buttable to 512 x 512). Counts integrated at pixel. No charge transfer! Developed at CERN for Medipix collaboration (xray) ~ 500 transistors/pixel
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First test detector Demountable detector
Simple lab vacuum, no photocathode Windowless – UV sensitive
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UV photon counting movie
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Sub-pixel spatial linearity
Lamp Pinhole Detector
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Imaged pinhole array Pinhole grid mask (0.5 x 0.5 mm) Gain: 20,000
Rear Field: 1600V Threshold: 3 ke- Gap: 500µm
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Avg. movement of 700 spots 1 pixel
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Position error (550 events/spot)
rms = 2.0 µm
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Vacuum Tube Design
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Vacuum Tube Design
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Vacuum Tube Design
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Vacuum Tube Design
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Medipix on a Header
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Summary Noiseless detectors outperform CCDs at low fluence per frame
Photocathode choice to fit application Medipix ASIC readout allows for a huge dynamic range, fast frame rate. MCP/Medipix Status First tube in Fall 2005 GaAs tube in 1st half of 2006
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Future Possibilities Medipix 3 now being discussed
130 nm CMOS technology Faster front end for less deadtime per pixel Faster readout rate (10 kHz frame rate) Radiation hard Si APDs rather than MCPs as photon converter/amplifier Higher optical QE Near IR response Cooling will be required to reduce dark count rate
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Acknowledgements This work was funded by an AODP grant managed by NOAO and funded by NSF Thanks to the Medipix Collaboration: Univ. of Barcelona University of Cagliari CEA CERN University of Freiburg University of Glasgow Czech Academy of Sciences Mid-Sweden University University of Napoli NIKHEF University of Pisa University of Auvergne Medical Research Council Czech Technical University ESRF University of Erlangen-Nurnberg
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Hexagonal multifiber boundaries
Flat Field MCP deadspots Hexagonal multifiber boundaries 1200 cts/bin - 500Mcps
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Histogram of Ratio consistent with counting statistics (2% rms)
Flat Field (cont) Histogram of Ratio consistent with counting statistics (2% rms) Ratio Flat1/Flat2
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256 bit fast shift register
Readout Architecture 3328 bit Pixel Column 0 3328 bit Pixel Column 255 3328 bit Pixel Column 1 256 bit fast shift register 32 bit CMOS output LVDS out Pixel values are digital (13 bit) Bits are shifted into fast shift register Choice of serial or 32 bit parallel output Maximum designed bandwidth is 100MHz Corresponds to 266µs frame readout
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256 bit fast shift register
3328 bit Pixel Column 0 3328 bit Pixel Column 255 3328 bit Pixel Column 1 256 bit fast shift register 32 bit CMOS output LVDS out
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“Built-in” Electronic Shutter
Enables/Disables counter Timing accuracy to 10 ns Uniform across Medipix Multiple cycles per frame No lifetime issues External input - can be phased to laser
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EUV and FUV ( nm)
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GaN UV Photocathodes, 100- 400 nm
The sensitivity of the activated photocathode is considerably higher, with a quantum efficiency of as high as 37% at about 450 Å and a sensitivity cut off energy of about 6.2 eV. The observed decrease of sensitivity at 988 and 520 Å (and probably not observed at ~670 Å) is likely to correspond to 2xEgap+Eaff,, 4xEgap+Eaff,, and 3xEgap+Eaff,, respectively. A much better spectral continuity of the illumination source is required in order to study the UV absorption fine structure.
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Hayashida et al. Beaune 2005 NIM
GaAsP Photocathodes Hayashida et al. Beaune 2005 NIM
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Avalanche Photodiodes (APDs, Geiger mode)
Single photon causes breakdown in over-voltaged diode QE potential of silicon Arrays in CMOS becoming available But Appreciable deadtime Low filling factor High dark counts, crosstalk and afterpulsing
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APD arrays 32 x 32 Edoardo Charbon
Ecole Polytechnique Federale de Lausanne
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L3CCD (e2V Technologies)
Integrates charge Multiplies charge in special readout register Adjust gain such that se < 1e- But Multiplication noise doubles photon noise variance Single readout limiting frame rate
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Assumed performance parameters
CCD Medipix-MCP Binning 2 x 2 6 x 6 8 x 8 QE (%) 90 35 Readout noise 2.5 e- Seeing width (pxls FWHM) 0.75 2.25 3 Diffract. width (pxls FWHM) 0.5 1.5 2
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Gaussian weighted center of gravity algorithm:
From Fusco et al SPIE , 2004
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Advantages of multi-pixel sampling of Shack-Hartmann spots
Non-linearity of 2 x 2 binning
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Advantages of multi-pixel sampling of Shack-Hartmann spots
Linear response off-null Insensitive to input width More sensitive to readout noise
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Technology advantage High QE CCDs Number of pixels CCDs, Medipix
Readout noise APD, Medipix, L3CCD Frame rate Medipix, CCD Gating Medipix
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Soft X-Ray Photocathodes
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