2010
DOI: 10.1117/12.857694
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Characterization and absolute QE measurements of delta-doped N-channel and P-channel CCDs

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Cited by 6 publications
(8 citation statements)
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“…At higher wavelengths or lower photon energies, the QY is approximately unity, and at wavelengths shorter than 360 nm 19 , this number is qualitatively proportional to the incident photon energies. This proportionality has been modeled and measured for higher photon energies including x-rays and has been reported for silicon by different groups as a constant number or as a function of incident photon energy [15,[19][20][21]. A detailed discussion can be found elsewhere [16,20,22].…”
Section: Resultsmentioning
confidence: 99%
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“…At higher wavelengths or lower photon energies, the QY is approximately unity, and at wavelengths shorter than 360 nm 19 , this number is qualitatively proportional to the incident photon energies. This proportionality has been modeled and measured for higher photon energies including x-rays and has been reported for silicon by different groups as a constant number or as a function of incident photon energy [15,[19][20][21]. A detailed discussion can be found elsewhere [16,20,22].…”
Section: Resultsmentioning
confidence: 99%
“…The uncoated region QE is in good agreement with the silicon transmittance data within the uncertainties of measurements. [12,16] The QY method used to determine the true QE, (i.e., fraction of photons detected) was direct measurement at each wavelength in our laboratory using the photon transfer technique [15,21]. of incident photons using two different QY sets of values to correct and normalize for multiple electrons per photon in the measured signal.…”
Section: Resultsmentioning
confidence: 99%
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“…Numerical simulations now predict that significant IGM gas accretion in cold (~10 4-5 K) flows fuels galaxy formation and on-going star formation in the early universe, perhaps extending to z=0 [9]. Amazingly, it is estimated that ~80% of the gravitational potential energy dissipated by the accreting gas may be radiated as Ly !…”
Section: ) Filament Correlationsmentioning
confidence: 99%
“…Antimony layers about 5 nm thick were applied in this way to 2k×4k and 1k×1k LBNL CCD's similar to those described here [64,65]. QE measurements with and without a (nominally) Si 3 N 4 /SiO 2 AR coating are shown in Ref.…”
Section: Prospects For Qe Improvementmentioning
confidence: 99%