Detectivity optimization to detect of ultraweak light fluxes with an EM-CCD as binary photon counter array

Abstract For a wide range of purposes, one faces the challenge to detect light from extremely faint and spatially extended sources. In such cases, detector noises dominate over the photon noise of the source, and quantum detectors in photon counting mode are generally the best option. Here, we combi...

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Autores principales: Ibtissame Khaoua, Guillaume Graciani, Andrey Kim, François Amblard
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Publicado: Nature Portfolio 2021
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Acceso en línea:https://doaj.org/article/28ded1f9c92a483683226f3d18576123
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spelling oai:doaj.org-article:28ded1f9c92a483683226f3d185761232021-12-02T12:09:05ZDetectivity optimization to detect of ultraweak light fluxes with an EM-CCD as binary photon counter array10.1038/s41598-021-82611-82045-2322https://doaj.org/article/28ded1f9c92a483683226f3d185761232021-02-01T00:00:00Zhttps://doi.org/10.1038/s41598-021-82611-8https://doaj.org/toc/2045-2322Abstract For a wide range of purposes, one faces the challenge to detect light from extremely faint and spatially extended sources. In such cases, detector noises dominate over the photon noise of the source, and quantum detectors in photon counting mode are generally the best option. Here, we combine a statistical model with an in-depth analysis of detector noises and calibration experiments, and we show that visible light can be detected with an electron-multiplying charge-coupled devices (EM-CCD) with a signal-to-noise ratio (SNR) of 3 for fluxes less than $$30\,{\text{photon}}\,{\text{s}}^{ - 1} \,{\text{cm}}^{ - 2}$$ 30 photon s - 1 cm - 2 . For green photons, this corresponds to 12 aW $${\text{cm}}^{ - 2}$$ cm - 2 ≈ $$9{ } \times 10^{ - 11}$$ 9 × 10 - 11 lux, i.e. 15 orders of magnitude less than typical daylight. The strong nonlinearity of the SNR with the sampling time leads to a dynamic range of detection of 4 orders of magnitude. To detect possibly varying light fluxes, we operate in conditions of maximal detectivity $${\mathcal{D}}$$ D rather than maximal SNR. Given the quantum efficiency $$QE\left( \lambda \right)$$ Q E λ of the detector, we find $${ \mathcal{D}} = 0.015\,{\text{photon}}^{ - 1} \,{\text{s}}^{1/2} \,{\text{cm}}$$ D = 0.015 photon - 1 s 1 / 2 cm , and a non-negligible sensitivity to blackbody radiation for T > 50 °C. This work should help design highly sensitive luminescence detection methods and develop experiments to explore dynamic phenomena involving ultra-weak luminescence in biology, chemistry, and material sciences.Ibtissame KhaouaGuillaume GracianiAndrey KimFrançois AmblardNature PortfolioarticleMedicineRScienceQENScientific Reports, Vol 11, Iss 1, Pp 1-11 (2021)
institution DOAJ
collection DOAJ
language EN
topic Medicine
R
Science
Q
spellingShingle Medicine
R
Science
Q
Ibtissame Khaoua
Guillaume Graciani
Andrey Kim
François Amblard
Detectivity optimization to detect of ultraweak light fluxes with an EM-CCD as binary photon counter array
description Abstract For a wide range of purposes, one faces the challenge to detect light from extremely faint and spatially extended sources. In such cases, detector noises dominate over the photon noise of the source, and quantum detectors in photon counting mode are generally the best option. Here, we combine a statistical model with an in-depth analysis of detector noises and calibration experiments, and we show that visible light can be detected with an electron-multiplying charge-coupled devices (EM-CCD) with a signal-to-noise ratio (SNR) of 3 for fluxes less than $$30\,{\text{photon}}\,{\text{s}}^{ - 1} \,{\text{cm}}^{ - 2}$$ 30 photon s - 1 cm - 2 . For green photons, this corresponds to 12 aW $${\text{cm}}^{ - 2}$$ cm - 2 ≈ $$9{ } \times 10^{ - 11}$$ 9 × 10 - 11 lux, i.e. 15 orders of magnitude less than typical daylight. The strong nonlinearity of the SNR with the sampling time leads to a dynamic range of detection of 4 orders of magnitude. To detect possibly varying light fluxes, we operate in conditions of maximal detectivity $${\mathcal{D}}$$ D rather than maximal SNR. Given the quantum efficiency $$QE\left( \lambda \right)$$ Q E λ of the detector, we find $${ \mathcal{D}} = 0.015\,{\text{photon}}^{ - 1} \,{\text{s}}^{1/2} \,{\text{cm}}$$ D = 0.015 photon - 1 s 1 / 2 cm , and a non-negligible sensitivity to blackbody radiation for T > 50 °C. This work should help design highly sensitive luminescence detection methods and develop experiments to explore dynamic phenomena involving ultra-weak luminescence in biology, chemistry, and material sciences.
format article
author Ibtissame Khaoua
Guillaume Graciani
Andrey Kim
François Amblard
author_facet Ibtissame Khaoua
Guillaume Graciani
Andrey Kim
François Amblard
author_sort Ibtissame Khaoua
title Detectivity optimization to detect of ultraweak light fluxes with an EM-CCD as binary photon counter array
title_short Detectivity optimization to detect of ultraweak light fluxes with an EM-CCD as binary photon counter array
title_full Detectivity optimization to detect of ultraweak light fluxes with an EM-CCD as binary photon counter array
title_fullStr Detectivity optimization to detect of ultraweak light fluxes with an EM-CCD as binary photon counter array
title_full_unstemmed Detectivity optimization to detect of ultraweak light fluxes with an EM-CCD as binary photon counter array
title_sort detectivity optimization to detect of ultraweak light fluxes with an em-ccd as binary photon counter array
publisher Nature Portfolio
publishDate 2021
url https://doaj.org/article/28ded1f9c92a483683226f3d18576123
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AT guillaumegraciani detectivityoptimizationtodetectofultraweaklightfluxeswithanemccdasbinaryphotoncounterarray
AT andreykim detectivityoptimizationtodetectofultraweaklightfluxeswithanemccdasbinaryphotoncounterarray
AT francoisamblard detectivityoptimizationtodetectofultraweaklightfluxeswithanemccdasbinaryphotoncounterarray
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