2006
DOI: 10.1016/j.infrared.2005.02.031
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Gas source MBE grown wavelength extended 2.2 and 2.5μm InGaAs PIN photodetectors

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Cited by 40 publications
(22 citation statements)
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“…In this case an additional buffer layer should be inserted to prevent the degradation of the photodetector performances. Wavelength-extended InGaAs photodiodes grown by hydride vapor phase epitaxy [4][5][6], metalorganic vapor phase epitaxy [7][8][9][10] or molecular beam epitaxy [11][12][13][14] methods with different buffer structures have been reported. In this article, the gas source molecular beam epitaxy (GSMBE) growth of InGaAs PIN photodetectors with cut-off wavelengths of 2.0, 2.4 and 2.7 mm at room temperature is reported and the effect of the buffer structure on the detector performance is investigated in detail.…”
Section: Introductionmentioning
confidence: 99%
“…In this case an additional buffer layer should be inserted to prevent the degradation of the photodetector performances. Wavelength-extended InGaAs photodiodes grown by hydride vapor phase epitaxy [4][5][6], metalorganic vapor phase epitaxy [7][8][9][10] or molecular beam epitaxy [11][12][13][14] methods with different buffer structures have been reported. In this article, the gas source molecular beam epitaxy (GSMBE) growth of InGaAs PIN photodetectors with cut-off wavelengths of 2.0, 2.4 and 2.7 mm at room temperature is reported and the effect of the buffer structure on the detector performance is investigated in detail.…”
Section: Introductionmentioning
confidence: 99%
“…The irradiation inducing degeneration of the performances of lattice-matched InGaAs detector has been studied in detail by http many researchers [7][8][9][10][11]. Extended wavelength InGaAs detectors attracted much attention in recent decades [2,[12][13][14][15]. However, the investigations on their irradiation effect are still far from enough.…”
Section: Introductionmentioning
confidence: 99%
“…Many efforts have been made to extend the cutoff wavelength of the In x Ga 1-x As photodetectors from about 1.7 lm (x = 0.53, lattice matched to InP substrate) to the longer wavelength side for the importance of the short wave infrared (SWIR) band of 1-3 lm [1][2][3][4][5][6][7][8][9][10][11], which exhibiting particular spectroscopic features including strong water absorption band around 1.4, 1.9 and 2.7 lm, as well as the high contrast for earth observation from the satellite [12]. However, to our knowledge the longest cutoff wavelength of the detectors at room temperature is still around 2.6-2.7 lm [2,11], which corresponding to a lattice mismatch of about 2.2% for x $ 0.85.…”
Section: Introductionmentioning
confidence: 99%