Far-Infrared Interferometry for Atomic Fine-Structure Line Observations

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[OIII] Ionization Sources[OIII] 88mm isabout 10 timesstronger than[NII] 122mm or[CII] 158mm allover the regionηCarKeyholeO 型星N. Smith et al 2004
Page 1 and 2: Far-Infrared Interferometry forAtom
Page 3 and 4: Atmospheric Transmission from Ataca
Page 5: Probe of Distant Universe• Hot Pl
Page 8 and 9: AzTEC-on-ASTEsurveys of SMGs
Page 10 and 11: • OIFIR atomic fine structure lin
Page 12 and 13: FIR SED ofStarburst galaxiesOI, OII
Page 14 and 15: The star formingregion IC1396 by th
Page 16: The Carina NebulaA very massive sta
Page 19 and 20: Carina Nebula by ISO LWS[CII]Mizuta
Page 21: [O III] 88mm & Ha
Page 25 and 26: [OIII] as a probe of highly ionized
Page 27 and 28: Transmittance1Dome_A_winter_75um0.8
Page 29 and 30: Antarctic THz Interferometer• Hig
Page 31 and 32: Direct detector vs. HeterodyneDirec
Page 34 and 35: MuFT andHeliostatin Nobeyama2005
Page 36: Subtraction of two output portsgive
Page 41: Summary• Probe of distant univers

Far-Infrared Interferometry for Atomic Fine-Structure Line Observations

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