Volume 532, August 2011
|Number of page(s)||41|
|Section||Interstellar and circumstellar matter|
|Published online||14 July 2011|
Comparison of the spectral survey lines with previous observations.
Comparison of the strong spectral survey lines simultaneously observed with different backends.
Identified non-blended lines. The line characteristics are derived from Gaussian fits.
© ESO, 2011
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