EDP Sciences
Free Access
Issue
A&A
Volume 577, May 2015
Article Number A72
Number of page(s) 11
Section Galactic structure, stellar clusters and populations
DOI https://doi.org/10.1051/0004-6361/201525815
Published online 06 May 2015

Online material

Table 1

Ages and masses determined by the SCEPtER pipeline.

thumbnail Fig. A.1

Top row: left Monte Carlo relative errors on mass estimate as a function of the true mass of the stars. The black lines show the position of the median (dashed line) and the 1σ envelope (solid line). The red lines show the corresponding quantities, but for weighted estimates. Right: same as in the left panel, but as a function of the relative age of the stars. Bottom row: same as the top row, but for age estimates.

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© ESO, 2015

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