Multiple-amplifier sensing charged-coupled device: model and improvement of the node removal efficiency

The multiple-amplifier sensing charge-coupled device (MAS-CCD) has emerged as a promising technology for astronomical observation, quantum imaging, and low-energy particle detection due to its ability to reduce the readout time for the same readout noise level compared with its predecessor, the skipper-CCD, by reading out the same charge packet through multiple inline amplifiers. Previous works identified a new parameter in this sensor, called node removal inefficiency (NRI), related to inefficiencies in charge transfer and residual charge removal from the sense node of each amplifier after readout. These inefficiencies can lead to distortions in the measured signals similar to those produced by the charge transfer inefficiencies in standard CCDs. We introduce more details in the mathematical model of the NRI mechanism and provide techniques to quantify its magnitude from the measured data. It also proposes a new operation strategy that significantly reduces its effect with minimal alterations of the timing sequences or voltage settings for the other signals of the sensor. The proposed technique is demonstrated experimentally on a 16-amplifier MAS-CCD. At the same time, the experimental data demonstrate that this approach minimizes the NRI effect to levels comparable with other sources of distortion such as the charge transfer inefficiency in scientific devices.

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Publication Details

Journal
Journal of Astronomical Telescopes Instruments and Systems
Published
2025-05-14
DOI
https://doi.org/10.1117/1.jatis.11.2.026004
Primary Topic
CCD and CMOS Imaging Sensors
Type
article
Field-Weighted Citation Impact
0.00

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article

Multiple-amplifier sensing charged-coupled device: model and improvement of the node removal efficiency

Agustín J. Lapi, Guillermo Fernández Moroni, Juan Estrada, Claudio Chavez et al.
3 links
Journal of Astronomical Telescopes Instruments and Systems
CCD and CMOS Imaging Sensors
article

Multiple-amplifier sensing charged-coupled device: model and improvement of the node removal efficiency

Agustín J. Lapi, Guillermo Fernández Moroni, Juan Estrada, Claudio Chavez, Fernando Chierchie, A. Drlica-Wagner, Blas J. Irigoyen Gimenez, Miqueas E. Gamero, Javier Tiffenberg
article en

Abstract

The multiple-amplifier sensing charge-coupled device (MAS-CCD) has emerged as a promising technology for astronomical observation, quantum imaging, and low-energy particle detection due to its ability to reduce the readout time for the same readout noise level compared with its predecessor, the skipper-CCD, by reading out the same charge packet through multiple inline amplifiers. Previous works identified a new parameter in this sensor, called node removal inefficiency (NRI), related to inefficiencies in charge transfer and residual charge removal from the sense node of each amplifier after readout. These inefficiencies can lead to distortions in the measured signals similar to those produced by the charge transfer inefficiencies in standard CCDs. We introduce more details in the mathematical model of the NRI mechanism and provide techniques to quantify its magnitude from the measured data. It also proposes a new operation strategy that significantly reduces its effect with minimal alterations of the timing sequences or voltage settings for the other signals of the sensor. The proposed technique is demonstrated experimentally on a 16-amplifier MAS-CCD. At the same time, the experimental data demonstrate that this approach minimizes the NRI effect to levels comparable with other sources of distortion such as the charge transfer inefficiency in scientific devices.

Journal of Astronomical Telescopes Instruments and SystemsVol. 11(02)
Fermi National Accelerator Laboratory (US), Universidad Nacional del Sur (AR)
Heising-Simons Foundation
Affordable and clean energy
Openalex Percentile: Top 91%
CCD and CMOS Imaging Sensors
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