2016
DOI: 10.1117/12.2233033
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RVS large format arrays for astronomy

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Cited by 8 publications
(5 citation statements)
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“…In the development of the pixel size and array size of HgCdTe FPA at Raytheon Vision Systems in recent years, it can be seen in Figure 3b that the detector pixel size has been reduced from the initial 61 µm to 20 µm, 8 µm, and 5 µm today. In contrast, the array sizes have been expanding from the initial 40 × 16, 64 × 64 to 2 K × 2 K, 4 K × 4 K, and even 8 K × 8 K nowadays, which shows the decreased pixel pitch and the increased array size [17,18]. Similarly, Raytron Technology [19] has successfully developed infrared detector chips with pixel size in a sequence of 35 Additionally, the overall area of the detector has not changed much.…”
Section: Lightweight and Miniaturizationmentioning
confidence: 99%
See 1 more Smart Citation
“…In the development of the pixel size and array size of HgCdTe FPA at Raytheon Vision Systems in recent years, it can be seen in Figure 3b that the detector pixel size has been reduced from the initial 61 µm to 20 µm, 8 µm, and 5 µm today. In contrast, the array sizes have been expanding from the initial 40 × 16, 64 × 64 to 2 K × 2 K, 4 K × 4 K, and even 8 K × 8 K nowadays, which shows the decreased pixel pitch and the increased array size [17,18]. Similarly, Raytron Technology [19] has successfully developed infrared detector chips with pixel size in a sequence of 35 Additionally, the overall area of the detector has not changed much.…”
Section: Lightweight and Miniaturizationmentioning
confidence: 99%
“…In other words, it can increase the number of focal plane pixels without changing the size area, thus increasing the resolution. [17,18].…”
Section: Lightweight and Miniaturizationmentioning
confidence: 99%
“…In a conventional source-follower HgCdTe array such as the Teledyne HxRG family 5 or the Raytheon Virgo, 6 there are two gains are of interest: the voltage gain (which has units of µV /ADU) and the charge gain (which has units of e − /ADU). The charge gain is related to the voltage gain through Q = CV where C is the integrating node capacitance (the sum of the photodiode and ROIC capacitances) and has a typical value of 20 to 40 f F .…”
Section: Avalanche Gain Charge Gain and The Excess Noise Factormentioning
confidence: 99%
“…While the operation of the SAPHIRA APD array is very similar to that of conventional HgCdTe arrays such as the Teledyne HAWAII series 5 and the Raytheon Virgo, 6 there are some important differences. The conventional arrays are normally operated at a bias of a few hundred mV , occasionally up to a volt, and the full bias voltage between the substrate and the node is within the dynamic range of the readout circuit.…”
Section: Introductionmentioning
confidence: 99%
“…The extrinsic doped p-on-n devices using arsenic doping technology that the preparation of p-n junction is realized by using arsenic ion implantation or in-situ doping have higher device performance, because the impurity concentration is controllable and has higher stability, and meanwhile, the influence of Hg vacancy on device performance is eliminated. RVS, TIS, AIM, Lynred (former Sofradir) and BAE have all adopted p-on-n device technology to develop high-performance HgCdTe infrared detectors [16][17][18][19][20][21][22][23][24] .…”
Section: Introductionmentioning
confidence: 99%