Far-Infrared Interferometry for Atomic Fine-Structure Line Observations

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Nobeyama Bolometer Array (NOBA)7-element NTD-Ge bolometersλ2 mm (150GHz)Operational since 1992Sunyaev-Zeldovich effectobserved with NOBA(Komatsu et al. 2001)
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 9 and 10: AzTEC/ASTE 1100um map of ADF-S (SEP
Page 11 and 12: Critical Density(cm -3 )[CII][NII][
Page 13 and 14: AKARI InfraredAstronomical Satellit
Page 15 and 16: Far-Infrared Surveyor (FIS)Martin-P
Page 18 and 19: ISO and AKARI observing points
Page 20 and 21: [C II] 158mm & HaN. Smith 2002
Page 22: [OIII] Ionization Sources[OIII] 88m
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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