Implementation of two multi-channel ASICs for CCD readout ASPIC (DSI design, LSST camera baseline) CLASSIC (Clamp & Sample design) ASICs designers : H. Lebboloa , R. Sefria , V. Tocutb Tests & Characterization : Pierre Antilogusa, S. Baileya, P. Baillya, J. Jeglotb, C.Juramya,, D. Martina , M. Moniezb ,F. Wicekb a IN2P3/LPNHE , b IN2P3/LAL LSST Focal Plane 189 Science CCD 4k X 4k 10mm pixels = 3 x109pixels for a focal plane of - 64 cm de diameter - 9.6 Deg 2 3X3 CCD “RAFT” The CCD are split in 16 segments of 1 M pixels : 2s readout time for the full focal plane => 500kHz Science Rafts (9 CCD): autonomous, fully testable 144 Mpixel camera. 1 Raft ~ 1/2 Megacam at CFHT LSST camera = 21 rafts 15/10/09 - Detectors for Astronomy 2009 Corner rafts : guiding and wavefront sensing ASICs for CCD readout 2 LSST camera readout system 189 Science CCD x 16 outputs = 3024 readout channels Request a compact readout chain inside the cryostat The topic of this talk : ASIC for FE CCD readout 15/10/09 - Detectors for Astronomy 2009 ASICs for CCD readout 3 LSST Front End : ASIC for CCD readout specifications Requirements : • CCD readout at 500 kHz (nominal) to 250 kHz • Noise : ~5nV / √Hz (or 7µV rms noise for 500ns integration ) ( ~2 e- to be compared to 5 e- read noise for the whole CCD Chain) • Power dissipation at cryo temperature : 20-25 mW/channel • Crosstalk : 10-4 level ( 0.01% (goal) - 0.05% (max) ) • 90Keˉ Full Well capacity (150Keˉ max) • 0.5% linearity ( defined over 0 to 100 000 eˉ full well ) • Differential outputs • Output Load : 50pF // 1 k Ω • Power Supply 0/5V with respect to reference = 2.5 V • Running temperature 173K Our initial worry : Does a 8 channels ASIC will have the required low level crosstalk 15/10/09 - Detectors for Astronomy 2009 ASICs for CCD readout 4 Analog signal processing of CCD : DSI or C&S The standard technique for analog signal processing of CCDs, is “Correlated Double Sampling”. It has been commonly implemented using one of the following schemes: • “Dual Slope Integrator” (DSI ) • “Clamp & Sample” (C&L) . Vout t reset feedthrough Reference level signal level Charge dump The first prototype implemented for LSST , the Analog Signal Processing ASic , (ASPIC I ), was a 8 channels ASIC with : • 4 DSI channels : The reference design for LSST is DSI. • 4 C&S channels : As we had a C&S design almost “ready” and considering the higher complexity of the DSI design and the R&D/unknown related to the crosstalk. 15/10/09 - Detectors for Astronomy 2009 ASICs for CCD readout 5 Analog signal processing of CCD : Dual Slope Integrator (DSI) Noise % 1/ sqrt (Tintegration) 5K 100pF 5K - 5K outp "diff DSI" outp inp + 10K + - Vref CDS 8k 2p 8p Vref (switches) 2k 10K 100pF Vref Vref - 5K inm "diff DSI" outm outm + Vref Clamp 1 gain , 2 integration constant time 15/10/09 - Detectors for Astronomy 2009 ASICs for CCD readout 6 Analog signal processing of CCD : Clamp and Sample (C&S) clamp Switch Noise % 1/ sqrt (Tau) With Tau = filter at the output of the C&S The “usage wants” Tau to be of the order 1/10 of the CCD signal width On ASPIC I , we had no filtering at the output of the C&S ( Tau ~ 35 ns ) 15/10/09 - Detectors for Astronomy 2009 ASICs for CCD readout 7 Analog signal processing of CCD :ASPIC I •Techno : CMOS 0.35µ 5V •Vendor : AMS •Package : CQFP100 TEST Require DSI C&S Crosstalk 0.05 % 0.007 % 0.02 % ~0.5% Goal 0.01% Linearity 0.5 % +/-0.2 % Power per channel 25 mW 48.5 mW (22o C) Noise 7 µV 19.04µV (Tint=500ns) 12µV (22o C) 10µV (-100o C) Cold Works at 100oC 24.3 mW 3.8mm ( -100oC) 4 DSI channels Tested down to -170oC 4 C&L channels 15/10/09 - Detectors for Astronomy 2009 ASICs for CCD readout 2.7mm 8 Analog signal processing of CCD : ASPIC I Conclusion The first prototype has demonstrated DSI and C&S : implementation in a multi channel Integrated Circuit work at low temperature with low crosstalk DSI : Good fit between measurements and simulations (based on an equivalent circuit using a linearized schematic to replace CDS switches) C&S : gave competitive results ASPIC II optimise Noise & Power and add functionalities Proto 1 - Noise density simulations & Measurements 50 45 DSI 40 µV 35 30 Noise measurement LPNHE 25 Noise measurement LAL 20 Noise simulation 15 10 5 0 0 0,05 15/10/09 - Detectors for Astronomy 2009 0,1 1/SQRT(Tint) 0,15 ASICs for CCD readout 9 Analog signal processing of CCD :ASPIC II 3 input amplifier gains : 2.5 – 5 – 7.5 to deal with CCD gain spread. 3 integration time constants : 500ns – 1µs – 1.5µs to deal with CCD readout frequency. Idle mode : DC current reduction by a factor of 1.000 •Techno : CMOS 0.35µ 5V •Vendor : AMS •Package : CQFP100 • 8 DSI channels baseline : { gain 5 + 500ns integration time} 15/10/09 - Detectors for Astronomy 2009 ASICs for CCD readout 10 ASPIC II : Layout and improvement LVDS inputs : 1.2V +/- 200mV terminated with 100 ohms CDS clocks: clamp + integrator reset + signal integration + reference integration CMOS inputs: 0V / +5V (compatible with 3.3V signals) input gain and integration time select Improvement compared to ASPIC I : Noise: 1/f noise reduced : amplifier first stage optimization RC Input gain : noise source Power consumption : Source identified : amplifier output stage. 15/10/09 - Detectors for Astronomy 2009 ASICs for CCD readout 11 ASPIC II : Simulation Noise simulations of ASPIC 2 @ -100°C 6µV RMS noise for an Integration Time of 500ns Noise 0.1% Linearity -0.15% 15/10/09 - Detectors for Astronomy 2009 ASICs for CCD readout 12 ASPIC II : first results TEST Require Crosstalk 0.05 % DSI (simul) DSI (measure) - 0.02 % Goal 0.01% Linearity 0.5 % Power per channel 25 mW Noise Goal 20 mW 7µV ( -100oC) 15/10/09 - Detectors for Astronomy 2009 +/-0.1 % +/-0.1% 25 mW (27o C) 20 mW(-100o C) 26 mW (22o C) 8 µV (27o C) 9 µV (22o C) (Tint=500ns) ASICs for CCD readout 13 “study on the side” : C&S version II ( CLASSIC ) • • • • • Pin to pin compatible with ASPIC 2 3 bit programmable gain input amplifier 4 bit programmable output time constant filter to match the readout frequency (tau = 8ns to 392ns ) Two differents C&S topologies (simulated noise ~ 1 efor a power < 20 mW/channel and 500 kHz CCD readout) Idle mode 15/10/09 - Detectors for Astronomy 2009 ASICs for CCD readout •Techno : CMOS 0.35µ 5V •Vendor : AMS •Package : CQFP100 • 8 C&S channels 14 Conclusion - - - We made a 8 channels ASICs with low crosstalk , low noise , low power, fast readout, for analog signal processing of CCD using CMOS 0.35µ 5V: - Such ASICs are needed for a large focal plane like the LSST one - If you are tired of fighting against « setup noise » , such ASIC with differential output directly in your cryostat could make your life so easier …. If you were expecting a “3 sigma effect” between DSI and C&S (or C&S and DSI) …looks like it was the wrong talk … still the difference is always in the detail ( crosstalk vs time , ultimate readout speed, connection to CCD …) , and we are far to have completed the characterization of our second generation of prototypes . For LSST, we now look forward to plug a LSST prototype CCD on our ASPIC II … 15/10/09 - Detectors for Astronomy 2009 ASICs for CCD readout 15