2011
DOI: 10.1109/tasc.2010.2090634
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Ultrawide Noise Bandwidth of NbN Hot-Electron Bolometer Mixers With In Situ Gold Contacts

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Cited by 9 publications
(6 citation statements)
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“…Generally, they are divided into low-temperature superconducting (LTS) and high-temperature superconducting (HTS) mixers based on the critical temperature of the superconducting materials. Typical LTS devices like superconductor-insulator-superconductor (SIS) mixers [4]- [6] and hot electron bolometer (HEB) mixers [7]- [9] are more sensitive than the HTS mixers, but they operate at liquid helium temperature (4.2 K) range thus requiring expensive and bulky cryogenic facilities. In comparison, the HTS devices operate at higher bath temperatures, where cheaper and portable single-stage cryocoolers can be used.…”
Section: Introductionmentioning
confidence: 99%
“…Generally, they are divided into low-temperature superconducting (LTS) and high-temperature superconducting (HTS) mixers based on the critical temperature of the superconducting materials. Typical LTS devices like superconductor-insulator-superconductor (SIS) mixers [4]- [6] and hot electron bolometer (HEB) mixers [7]- [9] are more sensitive than the HTS mixers, but they operate at liquid helium temperature (4.2 K) range thus requiring expensive and bulky cryogenic facilities. In comparison, the HTS devices operate at higher bath temperatures, where cheaper and portable single-stage cryocoolers can be used.…”
Section: Introductionmentioning
confidence: 99%
“…The transition temperature of a thin-lm superconductor depends on many parameters, including the transition temperature of the bulk superconductor, lm thickness, fabrication quality, and superconductor-substrate interface [77]. Some superconductors commonly used in HEB mixers are NbN [78][79][80][81], NbTiN [82][83][84] and Nb [85]. There are two mechanisms for cooling radiation-heated electrons: phononcooling and diffusion-cooling.…”
Section: Hot Electron Bolometer Mixersmentioning
confidence: 99%
“…For example, gure 7(a) shows an HEB mixer with an integrated planar spiral antenna, which is favorable for broadband operation [86]. DSB noise temperatures of 410 K at 0.8 THz [84], 490 K at 1.475 THz [87], 600 K at 2.5 THz [78], 1200 K at 3.1 THz [88], 1300 K at 4.3 THz [79], 815 K at 4.7 THz [80], and 1520 K at 5.2 THz [81] have been demonstrated using HEB mixers. HEB mixers have been successfully employed in many missions, including the APEX Telescope [89], HIFI [69], and GREAT [90].…”
Section: Hot Electron Bolometer Mixersmentioning
confidence: 99%
“…There are many types of cryogenic THz detectors: indium antimonide hot electron bolometers [13,14,15], quantum well infrared detectors [16,17,18], superconducting bolometers [19,20,21] or doped germanium bolometers [22,23,24]. In the present paper, we consider a detector based on an epitaxial layer of HgCdTe.…”
Section: Introductionmentioning
confidence: 99%