Abstract

Lynx requires large-format x-ray imaging detectors with performance at least as good as the best current-generation devices but with much higher readout rates. We are investigating an advanced charge-coupled device (CCD) detector architecture under development at MIT Lincoln Laboratory for use in the Lynx high-definition x-ray imager and x-ray grating spectrometer instruments. This architecture features a CMOS-compatible detector integrated with parallel CMOS signal processing chains. Fast, low-noise amplifiers and highly parallel signal processing provide the high frame rates required. CMOS-compatibility of the CCD enables low-power charge transfer and signal processing. We report on the performance of CMOS-compatible test CCDs read at pixel rates up to 5.0 Mpix s − 1 (50 times faster than Chandra ACIS CCDs), with transfer clock swings as low as 1.0-V peak-to-peak (power/gate-area comparable to ACIS CCDs at 100 times the parallel transfer rate). We measure read noise of 4.6 electrons RMS at 2.5 MHz and x-ray spectral resolution better than 150-eV full-width at half maximum at 5.9 keV for single-pixel events. We report charge transfer efficiency measurements and demonstrate that buried channel trough implants as narrow as 0.8 μm are effective in improving charge transfer performance. We find that the charge transfer efficiency of these devices drops significantly as detector temperature is reduced from ∼ − 30 ° C to −60 ° C. We point out the potential of previously demonstrated curved-detector fabrication technology for simplifying the design of the Lynx high-definition imager. We discuss the expected detector radiation tolerance at these relatively high transfer rates. Finally, we note that the high pixel “aspect ratio” (depletion depth: pixel size ≈9 ∶ 1) of our test devices is similar to that expected for Lynx detectors and discuss implications of this geometry for x-ray performance and noise requirements.

Highlights

  • Two decades after the launch of Chandra and XMM/ Newton, a new generation of large, scientifically ambitious, and exciting x-ray astrophysics missions is being planned

  • We describe an advanced charge-coupled device (CCD) technology we are developing in part to meet the requirements of the Lynx high-definition x-ray imager4 (HDXI) and x-ray grating spectrograph (XGS)

  • We first present CCID93 amplifier performance and x-ray spectral resolution measurements obtained at MIT Kavli Institute (MKI) and discuss charge transfer performance measurements obtained at both Lincoln and MKI

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Summary

Introduction

Two decades after the launch of Chandra and XMM/ Newton, a new generation of large, scientifically ambitious, and exciting x-ray astrophysics missions is being planned. The second path aims to develop compact, highly parallel signal processing chains allowing high frame rates with modest analog-to-digital conversion rates When fully demonstrated, these two technologies will be combined, first as discrete elements, and potentially as a single-detector module by means, for example, of three-dimensional integration of analog and digital tiers through hybrid wafer bonding. We describe an advanced charge-coupled device (CCD) technology we are developing in part to meet the requirements of the Lynx HDXI and XGS This “digital CCD” (DCCD) technology aims to provide the proven spectroscopic performance of conventional x-ray CCD detectors in a CMOS-compatible sensor capable of much higher frame rates with much lower power consumption. We conclude with a summary and discussion of our near-term development plans

Overview
Single-Level Polysilicon Transfer Gates
Test Devices
Test Results
CCID93 amplifier performance and x-ray spectral resolution
CCID93 charge transfer performance
Lynx HDXI Focal Plane
Radiation Tolerance
Charge Collection
Summary and Plans

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