2021
DOI: 10.1109/jqe.2021.3087324
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High Temperature Behaviors of 1–2.5 μm Extended Wavelength In₀.₈₃Ga₀.₁₇As Photodetectors on InP Substrate

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Cited by 6 publications
(4 citation statements)
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“…This is partially because the smaller wavenumbers are more vulnerable to detector response variations due to thermal fluctuations, since the detector has a large slope around 3850 cm -1 , and thermal fluctuations cause this slope to shift around this value changing the PSD value. 29 To isolate the effects of drift and noise, the data are fitted to a custom equation that captures most of its variation. The fitting equation depends on the wavenumber.…”
Section: Resultsmentioning
confidence: 99%
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“…This is partially because the smaller wavenumbers are more vulnerable to detector response variations due to thermal fluctuations, since the detector has a large slope around 3850 cm -1 , and thermal fluctuations cause this slope to shift around this value changing the PSD value. 29 To isolate the effects of drift and noise, the data are fitted to a custom equation that captures most of its variation. The fitting equation depends on the wavenumber.…”
Section: Resultsmentioning
confidence: 99%
“…This is partially because the smaller wavenumbers are more vulnerable to detector response variations due to thermal fluctuations, since the detector has a large slope around 3850 cm –1 , and thermal fluctuations cause this slope to shift around this value changing the PSD value. 29…”
Section: Resultsmentioning
confidence: 99%
“…Otherwise, the spectra response range is the primary parameter for SWIR photodetection, which always requires a narrow bandgap and wide spectra adsorption [11][12][13][14][15][16]. Hence, high mobility, high quality, and wide spectra response are key factors for the next generation of SWIR photodetectors with high temperature tolerance [17][18][19][20].…”
Section: Introductionmentioning
confidence: 99%
“…Utilizing commercial InGaAs material to operate in the 1.7-μm to 2-μm wavelength band poses very challenging issues which are exacerbated for wavelengths longer than 2 μm because state-of-the-art strained InGaAs devices, when compared to their lattice-matched (to InP) counterparts with a cut-off wavelength of 1.7 μm, suffer from high defect densities, lower detectivity and higher dark currents, and thus need cryogenic cooling to improve performance. [15][16][17][18] Furthermore, a severe reduction of QE in extended InGaAs is observed that has been attributed to the relatively large band offsets present in heterojunction architectures that are usually employed to reduce Shockley-Read-Hall (SRH) junction dark current. [19][20][21][22] While HgCdTe SWIR photodetectors have shown remarkable performance levels, the reported devices appear to be based on MWIR device designs in which the absorber composition has been tailored to the desired SWIR cut-off wavelength.…”
Section: Introductionmentioning
confidence: 99%