Code for CMOS Dark Current Noise Modelling and Bad Pixel Detection
Peng Jia
The code uses the clustering method to build response matrix of each pixel in the CMOS according to the ground test data, which could be used for different CMOS cameras in satellites.
Files
Code-A Data-Driven Approach for Mitigating Dark Current Noise and Bad Pixels in Complementary Metal Oxide Semiconductor Cameras for Space-based Telescopes.zip
5.76 kB
Paper Information
Paper Title:
A Data-Driven Approach for Mitigating Dark Current Noise and Bad Pixels in Complementary Metal Oxide Semiconductor Cameras for Space-based Telescopes
Publication:
AJ
Identifiers
CSTR:
11379.19.101387
DOI:
10.12149/101387
VO Identifier:
ivo://China-VO/paperdata/101387
Publication Date:
2024-03-15
Citation Guidelines
Peng Jia et al. 2024. Code for CMOS Dark Current Noise Modelling and Bad Pixel Detection. Version 1.0. https://doi.org/10.12149/101387
@misc{10.12149/101387,
doi = {10.12149/101387},
url = {https://doi.org/10.12149/101387},
author = {Peng Jia},
title = {Code for CMOS Dark Current Noise Modelling and Bad Pixel Detection},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2024}
}
doi = {10.12149/101387},
url = {https://doi.org/10.12149/101387},
author = {Peng Jia},
title = {Code for CMOS Dark Current Noise Modelling and Bad Pixel Detection},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2024}
}
Versions
Main
This DOI represents all versions, and will always resolve to the latest one.
2024-03-15