Far-Infrared Interferometry for Atomic Fine-Structure Line Observations

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30Dor region andR136Figure is deleted.[OIII] distributed 150 pc around R136[OIII] 88mm isobserved widelydistributed aroundR136Contour: MIPS 24mmred: O and WR starsKawada et a. (2010)
[OIII] as a probe of highly ionized gasHigh-mass star-forming regionProbe of FUV radiation and electron densityDetailed observation of nearby galaxiesInitial burst of star-formationALMA will observe [OIII] in z > 6 universeGamma-ray burst and star-forming galaxies at z > 8Observe the site of cosmic re-ionizationLet’s start with the Antarctica THz Interferometer !
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 and 22: [O III] 88mm & Ha
Page 26 and 27: Antarctic TerahertzInterferometer
Page 28 and 29: FIR atomic fine structure lines•
Page 30 and 31: NEFD [Jy sqrt s]Comparison of Sensi
Page 32: FTS measurement ofatmospheric trans
Page 35 and 36: MuFT image of the sunA. baselines s
Page 40 and 41: Space THz InterferometerThe Road Ma

Far-Infrared Interferometry for Atomic Fine-Structure Line Observations

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