Comparative modelling of the spectra of cool giants

Free Access

Issue		A&A Volume 547, November 2012


Article Number		A108
Number of page(s)		30
Section		Stellar atmospheres
DOI		https://doi.org/10.1051/0004-6361/201219142
Published online		06 November 2012

Online material

Table 6

Iron line selection for the M6 stellar parameter determination (Sect. 3.1.6).

Table 7

Lines used in the A1 analysis to determine abundances for Star 1.

Table 8

Fe I lines used in the A1 analysis to determine iron abundances for Star 3.

Table 9

Lines used by the A2 participants (Sect. 3.2.2).

Table 10

Lines analysed by A5 (Sect. 3.2.5).

Table 11

Measured CO 3–0 lines in Star 4 from the T analysis (Sect. 3.5).

© ESO, 2012

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