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Documents SiO J=5-4 in the HH211 Protostellar Jet Imaged with the SMA Naomi Hirano (ASIAA, Taiwan) (=^_^=)...

Slide 1 SiO J=5-4 in the HH211 Protostellar Jet Imaged with the SMA Naomi Hirano (ASIAA, Taiwan) (=^_^=) (=^_^=)/ Sheng-yuan Liu 1, Hsien Shang 1, PaulT.P. Ho 2, Hui-Chun…

Documents Spectral Line Observing I

Introduction Most of what you have heard about so far has applied to a single spectral channel with some frequency width, dn Many astronomical problems require many channels…

Documents Calibration, Imaging and Analysis of Data Cubes

Outline Why spectral line (multi-channel) observing? Not only for spectral lines, but there are many advantages for continuum experiments as well Calibration specifics Bandpass,…

Documents Star and Planet Formation

Star and Planet Formation Sommer term 2007 Henrik Beuther & Sebastian Wolf 16.4 Introduction (H.B. & S.W.) 23.4 Physical processes, heating and cooling, radiation…

Documents Twelfth Synthesis Imaging Workshop 2010 June 8-15 Calibration, Imaging and Analysis of Data Cubes...

Outline Why spectral line (multi-channel) observing? Not only for spectral lines, but there are many advantages for continuum experiments as well Calibration specifics Bandpass,…