| Issue |
A&A
Volume 550, February 2013
|
|
|---|---|---|
| Article Number | A125 | |
| Number of page(s) | 16 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/201117747 | |
| Published online | 06 February 2013 | |
Online material
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Fig. 7
Evolution of the bias (black crosses) and dispersion (red asterisks) of the MATISSE atmospheric parameters for synthetic spectra (at SNR = 10) of 2000 stars randomly chosen in the LRc01 BGM request. |
| Open with DEXTER | |
 |
Fig. 9
Distribution of the stellar distances for our observed sample (red dashed line) and the BGM1 simulation (blue). The error bars correspond to 1σ of the Gaussian function fitting the distribution of the corresponding bin. |
| Open with DEXTER | |
 |
Fig. 10
Distribution of the metallicity for our observed sample (red dashed line) and the BGM1 simulation (blue). The error bars correspond to 1σ of the Gaussian function fitting the distribution of the corresponding bin. |
| Open with DEXTER | |
 |
Fig. 11
Kinematic comparison (three velocity components) of our observed sample with the BGM1 simulations for the three CoRoT fields. The observations are represented with a red dashed line and the BGM1 data with a solid blue line. |
| Open with DEXTER | |
© ESO, 2013
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