1998
DOI: 10.1109/23.682658
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The depletion depth of high resistivity X-ray CCDs

Abstract: We have developed several techniques which allow measurement of the depletion depth of X-ray CCDs used for imaging and spectroscopy in the 0.2 -10 keV energy band. These methods were developed as part of the calibration program for the AXAF CCD Imaging Spectrometer (ACIS). The depletion depth is a parameter that determines the high-energy detection limit of the CCDs. One technique is based on the analysis of long traces of high energy ionizing particles traveling through the CCD nearly parallel to its surface.… Show more

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Cited by 8 publications
(4 citation statements)
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“…We have determined the backside voltage needed to fully deplete the 100 micron region for the TESS CCDs is approximately −20V. This was verified two ways: high energy cosmic rays produce diffusion clouds along the entire path as they travel from one surface of the detector to the opposite one through the bulk of the substrate, and show a characteristic wide plume if the device has an undepleted portion [5]. A trail that is narrow along its entire length indicates that the electric field is present everywhere, and the detector is fully depleted; an example of such a trail is shown in figure 1.…”
Section: Back Side Depletionmentioning
confidence: 77%
“…We have determined the backside voltage needed to fully deplete the 100 micron region for the TESS CCDs is approximately −20V. This was verified two ways: high energy cosmic rays produce diffusion clouds along the entire path as they travel from one surface of the detector to the opposite one through the bulk of the substrate, and show a characteristic wide plume if the device has an undepleted portion [5]. A trail that is narrow along its entire length indicates that the electric field is present everywhere, and the detector is fully depleted; an example of such a trail is shown in figure 1.…”
Section: Back Side Depletionmentioning
confidence: 77%
“…For BI CCDs, both subgroup event percentage and mean PIP shift depend sensitively on energy, at low energy (E < 2 keV); however, the three subgroups of splitevent percentages and PIP shifts are insensitive to energy for E > 6 keV. This reflects the fact that, for photons with energy exceeding 6 keV, the characteristic penetration depth becomes comparable to or larger than the thickness of the ACIS BI CCD, which is only 45 m. In contrast, ACIS FI CCDs are much thicker, with larger depletion depth ($70 m; Prigozhin et al 1998a). Therefore, the branching ratios and PIP shifts depend sensitively on energy over most of the Chandra ACIS bandwidth.…”
Section: Energg Y-dependent Ser For Fi Ccdsmentioning
confidence: 79%
“…The detailed explanation of these structures is shown in Table 1. To reverse-bias the photodiode, 400 V is applied at the bottom contact of the N-type Si substrate [20]. Under such a high reverse-bias voltage, full depletion can be achieved in the Si substrate.…”
Section: Pixel Structurementioning
confidence: 99%