Free Access
Volume 532, August 2011
Article Number A23
Number of page(s) 41
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/201015399
Published online 14 July 2011

Online material

Table 2

Comparison of the spectral survey lines with previous observations.

Table 3

Comparison of the strong spectral survey lines simultaneously observed with different backends.

Table 4

Identified non-blended lines. The line characteristics are derived from Gaussian fits.

© ESO, 2011

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