... systems

The data base is available at CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/366/538

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... BaSeL-2.2

The BaSeL-1.0 and BaSeL-2.0 libraries were published in Lejeune et al. (1997) and Lejeune et al. (1998) respectively, while BaSeL-2.2 is available only electronically at ftp://ftp.astro.unibas.ch/pub/lejeune/. See also this ftp site for a description of the changes in the different versions.

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... 3.5

In the previous versions of the BaSeL models, we adopted $T_{\rm eff}$ = 5000 K and $\log g$ = 2.5 as the upper limits for the calibration of giants (see Lejeune et al. 1998 for details).

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... ${\rm [Fe/H]}$

The solar metallicity ${\rm [Fe/H]}$ =0 is identified with the Z=0.02 tracks. For other metallicities, we adopt the relation $\mathrm{[Fe/H]} \equiv \log(Z/Z_{\odot})$, with $Z_{\odot}= 0.02$.

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...=0.0

To avoid the confusion with the Johnson V band, the Geneva V^* is noted with an asterisk hereafter.

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... responses

The tables can be retrieved from the STScI ftp site ( ftp://ftp.stsci.edu/cdbs/cdbs8/synphot_tables/) as files pcfxxxwsys.txt, where xxx designates the mean filter wavelength in nm.

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... CDS

http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/
366/538

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