Aug 2026· Astronomical Telescopes + Instrumentation· Vol 14157, pp. 141570G - 141570G-6· 1 citation· 13 references
Engineering
Abstract
To meet the requirements of future high-throughput and high spatial resolution Lynx-like X-ray observatories, the Pennsylvania State University High-Energy Astrophysics Detector and Instrumentation Lab, in collaboration with Teledyne Imaging Sensors (TIS), has developed a next-generation small-pixel soft X-ray hybrid CMOS detector (HCD). The Small-Pixel-1024 is an HCD with a 1024×1024 grid of 12.5-micron pitch pixels, featuring a high-gain capacitive transimpedance amplifier and in-pixel correlated double sampling. The Small-Pixel-1024 can operate in full-frame and windowed modes, with full-frame readout speeds up to 149 frames/s and windowed readout rates exceeding 1 kHz. For development efforts, two separate pixel designs were created using different feedback capacitance circuit schemes to restore pixel full-well post pixel reset, allowing for X-ray sensitivity up to 20 keV. The ‘A0’ pixels use a capacitor that can be enabled or disabled and retains heritage from a prototype small-pixel detector. The ‘A1’ pixels use the more traditional CMOS scheme of a complementary passgate that cannot be disabled. Here, we report on the methods and results for the characterization and optimization of the Small-Pixel-1024 dark current, read noise, gain variation, and energy resolution, including a comparison between the two pixel types.
Recent developments in particle physics require cost-effective pixel detectors capable of operating under increased energy and luminosity conditions foreseen in future collider experiments. In response, monolithic CMOS pixel sensors incorporating modern readout architectures have emerged, combining high-rate capability...
M. M. Ameen, G. Dash, A. Vijay et al.· Physics· 0 citations
Time projection chambers equipped with gas electron multipliers and optical readout by scientific CMOS cameras are a promising technology for low-energy particle detection, as demonstrated by the CYGNO experiment. To help identify an optimal detector configuration, we performed a characterization of two state-of-the-ar...
B. D. Almeida, F. D. Amaro, R. Antonietti et al.· Measurement science and tech...· 2 citations
The far-infrared (FIR) foreground level in space is extremely low, necessitating highly sensitive detectors for space-based continuum observations. To achieve photon-noise-limited performance, FIR detectors require a noise equivalent power (NEP) lower than 3×10 -19 W/Hz 1/2 and a per-pixel saturation power (P sat ) r...
Ling-Mei Zhang, Jia-Min Sun, Lin Zhu et al.· Superconductors Science and...· 0 citations
Multi-gap Resistive Plate Chamber (MRPC) detectors offer excellent time resolution and detection efficiency, creating a strong demand for high-precision, highly scalable timing readout systems. In this work, a readout electronics system is designed for a large-area 100*100 cm MRPC detector containing 2400 high-granular...
Digital silicon photomultipliers (dSiPM) are arrays of single photon avalanche diodes (SPADs) where each SPAD has its own electronic readout. To maximize the photodetection area, we developed a readout integrated circuit (ROIC) 3D-integrated to a custom-designed SPAD layer fabricated at Teledyne Dalsa (Bromont, Canada)...
O. Lepage, T. Rossignol, N. Roy et al.· Journal of Instrumentation· 1 citation
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