Free Access
Issue
A&A
Volume 520, September-October 2010
Article Number A85
Number of page(s) 17
Section Stellar atmospheres
DOI https://doi.org/10.1051/0004-6361/200912894
Published online 07 October 2010

Online Material

Appendix A: Spectral fits

\begin{figure}
\begin{flushleft}
In this section, the best fits are shown for ea...
...}\vspace*{3mm}
\par\includegraphics[width=8.8cm,clip]{12894fgA1.ps}
\end{figure} Figure A.1:

Upper panel: observed spectrum (black line) for the cluster HW1 and the best model fitted by S TARLIGHT+PEGASE-HR (blue line). Lower panel: residuals of the fit.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA2.ps}
\end{figure} Figure A.2:

Same as Fig. A.1 for cluster K3 (ESO).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA3.ps}
\end{figure} Figure A.3:

Same as Fig. A.1 for cluster K3 (LNA).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA4.ps}
\end{figure} Figure A.4:

Same as Fig. A.1 for cluster L3.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA5.ps}
\end{figure} Figure A.5:

Same as Fig. A.1 for cluster L11.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA6.ps}
\end{figure} Figure A.6:

Same as Fig. A.1 for cluster L113.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA7.ps}
\end{figure} Figure A.7:

Same as Fig. A.1 for cluster NGC 121 (ESO).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA8.ps}
\end{figure} Figure A.8:

Same as Fig. A.1 for NGC 121 (LNA).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA9.ps}
\end{figure} Figure A.9:

Same as Fig. A.1 for cluster NGC 152.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA10.ps}
\end{figure} Figure A.10:

Same as Fig. A.1 for cluster NGC 222.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA11.ps}
\end{figure} Figure A.11:

Same as Fig. A.1 for cluster NGC 256.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA12.ps}
\end{figure} Figure A.12:

Same as Fig. A.1 for cluster NGC 269.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA13.ps}
\end{figure} Figure A.13:

Same as Fig. A.1 for cluster NGC 294.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA14.ps}
\end{figure} Figure A.14:

Same as Fig. A.1 for cluster NGC 361 (ESO99).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA15.ps}
\end{figure} Figure A.15:

Same as Fig. A.1 for NGC 361 (ESO00).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA16.ps}
\end{figure} Figure A.16:

Same as Fig. A.1 for cluster NGC 419.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA17.ps}
\end{figure} Figure A.17:

Same as Fig. A.1 for cluster NGC 458.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA18.ps}
\end{figure} Figure A.18:

Upper panel: observed spectrum (black line) for the cluster HW1 and the best model fitted by ULySS+PEGASE-HR (blue line). Red pixels correspond to regions of telluric lines and were rejected from the fit. Lower panel: residuals of the fit. The continuous green lines mark the 1-$\sigma $ deviation.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA19.ps}
\end{figure} Figure A.19:

Same as Fig. A.18 for cluster K3 (ESO).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA20.ps}
\end{figure} Figure A.20:

Same as Fig. A.18 for cluster K3 (LNA).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA21.ps}
\end{figure} Figure A.21:

Same as Fig. A.18 for cluster L3.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA22.ps}
\end{figure} Figure A.22:

Same as Fig. A.18 for cluster L11.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA23.ps}
\end{figure} Figure A.23:

Same as Fig. A.18 for cluster L113.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA24.ps}
\end{figure} Figure A.24:

Same as Fig. A.18 for cluster NGC 121 (ESO).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA25.ps}
\end{figure} Figure A.25:

Same as Fig. A.18 for NGC 121 (LNA).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA26.ps}
\end{figure} Figure A.26:

Same as Fig. A.18 for cluster NGC 152.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA27.ps}
\end{figure} Figure A.27:

Same as Fig. A.18 for cluster NGC 222.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA28.ps}
\end{figure} Figure A.28:

Same as Fig. A.18 for cluster NGC 256.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA29.ps}
\end{figure} Figure A.29:

Same as Fig. A.18 for cluster NGC 269.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA30.ps}
\end{figure} Figure A.30:

Same as Fig. A.18 for cluster NGC 294.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA31.ps}
\end{figure} Figure A.31:

Same as Fig. A.18 for cluster NGC 361 (ESO99).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA32.ps}
\end{figure} Figure A.32:

Same as Fig. A.18 for NGC 361 (ESO00).

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA33.ps}
\end{figure} Figure A.33:

Same as Fig. A.18 for cluster NGC 419.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=8.8cm,clip]{12894fgA34.ps}
\end{figure} Figure A.34:

Same as Fig. A.18 for cluster NGC 458.

Open with DEXTER

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