2019
DOI: 10.1016/j.optcom.2018.12.061
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Intensity modulation-based spectral polarization measurement method of coded aperture

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Cited by 16 publications
(6 citation statements)
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“…This limits its use for large scale scenes because of the expensive computational memory requirements and the potential overfitting problems [64]. We propose to reduce the number of trainable parameters by adding spatial structure to each CA so that a kernel Q s of size ∆ n × ∆ m N × M is periodically repeated as follows Number of snapshots in (10) Trainable parameters in (14) manufacturing noise in (16) Conditionality in (13) Multishot correlation in (12) 4. Regularizer Fig.…”
Section: F Data Driven Conditionality Constraintmentioning
confidence: 99%
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“…This limits its use for large scale scenes because of the expensive computational memory requirements and the potential overfitting problems [64]. We propose to reduce the number of trainable parameters by adding spatial structure to each CA so that a kernel Q s of size ∆ n × ∆ m N × M is periodically repeated as follows Number of snapshots in (10) Trainable parameters in (14) manufacturing noise in (16) Conditionality in (13) Multishot correlation in (12) 4. Regularizer Fig.…”
Section: F Data Driven Conditionality Constraintmentioning
confidence: 99%
“…This numerical test aims to demonstrate the importance of reducing the number of trainable parameters to avoid overffiting problems in the E2E approach by using the CA structure strategy presented in (14). For this, we select the CASSI system, with 5 < (L = 31) optical filters in the Colored-CA, for the reconstruction task.…”
Section: G Number Of Trainable Parameters Experimentsmentioning
confidence: 99%
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“…The spectropolarimetric resolution recovered from the CS and CSIM retains the intrinsic spectral resolution of the imaging spectrometer used. This point is very important for the imaging spectrometers that only have modest spectral resolution 12 , 19 , 31 , 32 . However, the FTM, CS, and CSIM methods are still subject to noise perturbation, since the SPI systems usually have lower flux due to a narrow spectral band and the use of a polarizer.…”
Section: Introductionmentioning
confidence: 99%
“…This point is very important for the imaging spectrometers that only have modest spectral resolution. 12,19,31,32 However, the FTM, CS, and CSIM methods are still subject to noise perturbation, since the SPI systems usually have lower flux due to a narrow spectral band and the use of a polarizer. In addition, the FTM and CS methods are enslaved to systematic errors originating from double MORs.…”
Section: Introductionmentioning
confidence: 99%