Presentation	2000/6/23 SANE2000-29 An SIS receiver on the Mt.Fuji submillimeter-wave telescope Yutaro Sekimoto,
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Abstract(in English)	We have developed a 1.2m submillimeter-wave telescope at the summit of Mt. Fuji to survey emission lines of the neutral carbon atom(492GHz)toward the Milky Way. A superconductor-insulator-superconductor(SIS) mixer receiver on the Nasmyth focus is used to observe the 800 / 500 / 350GHz bands, simultaneously. The receiver noise temperature is 100K at 350GHz, 120K at 500GHz, and 600k at 800GHz.
Keyword(in Japanese)	(See Japanese page)
Keyword(in English)	submillimeter-wave receiver / submillimeter-wave telescope / submillimeter-wave astronomy / Heterodyne receiver / Neutral carbon atom
Paper #	SANE2000-29
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Conference Information
Committee	SANE
Conference Date	2000/6/23(1days)
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Paper Information
Registration To	Space, Aeronautical and Navigational Electronics (SANE)
Language	JPN
Title (in Japanese)	(See Japanese page)
Sub Title (in Japanese)	(See Japanese page)
Title (in English)	SANE2000-29 An SIS receiver on the Mt.Fuji submillimeter-wave telescope
Sub Title (in English)
Keyword(1)	submillimeter-wave receiver
Keyword(2)	submillimeter-wave telescope
Keyword(3)	submillimeter-wave astronomy
Keyword(4)	Heterodyne receiver
Keyword(5)	Neutral carbon atom
1st Author's Name	Yutaro Sekimoto
1st Author's Affiliation	Nobeyama Radio Observatory, National Astronomical Observatory of Japan()
Date	2000/6/23
Paper #	SANE2000-29
Volume (vol)	vol.100
Number (no)	162
Page	pp.pp.-
#Pages	6
Date of Issue