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Matches in SemOpenAlex for { <https://semopenalex.org/work/W1998129431> ?p ?o ?g. }

• W1998129431 endingPage "958" @default.
• W1998129431 startingPage "951" @default.
• W1998129431 abstract "We have developed a low-noise submillimeter-wave SIS receiver (320–360 GHz) for a 10 m submillimeter telescope, which was installed at Nobeyama in 2000 February. This receiver and a millimeter-wave SIS receiver are mounted on the ceiling of the Cassegrain receiver cabin of the 10 m telescope. Two curved mirrors couple a shaped Cassegrain beam from the subreflector to mixer horns. The minimum noise temperature measured in front of the receiver was 52 K in double sideband (DSB) at a local oscillator (LO) frequency of 354 GHz, which corresponds to three-times quantum limits (⁠|$3hnu/k_{mathrm{B}}$|⁠). This noise temperature contributions are resolved into the optics, mixer, and IF parts. The temperature ripple of a two-stage Gifford–McMahon cryocooler has been reduced to be 2 mK peak-to-peak at the mixer block with a helium pot temperature stabilizer. Mechanical vibration (30 |${mu mathrm {m}}$| peak-to-peak) of the cold head degrades the receiver stability." @default.
• W1998129431 created "2016-06-24" @default.
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• W1998129431 date "2001-10-25" @default.
• W1998129431 modified "2023-10-15" @default.
• W1998129431 title "A 350 GHz SIS Receiver on the Nobeyama 10 m Submillimeter Telescope" @default.
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• W1998129431 doi "https://doi.org/10.1093/pasj/53.5.951" @default.
• W1998129431 hasPublicationYear "2001" @default.
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