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Table 1

AV, Vlim, and MVlim for all samples at the bright (min) and faint (max) ends.

MB EC

In All In All

S1 S2 CS S1 S2 CS S1 S2 CS S1 S2 CS

11

16.7 16.7 16.3 15.7 15.7 15.3 16.7 16.7 16.3 15.7 15.7 15.3

AVmin(1.2kpc) 1.5 1.8
AVmax(3kpc) 3.1 3.2
MVlim(1.2kpc) –0.9 –1.2
SPmin B4 B3.5

MVlim(3kpc) 1.2 1.2 0.8 0.2 0.2 –0.2 1.1 1.1 0.7 0.1 0.1 –0.3
SPmax A1 A1 A0 B8.5 B8.5 B7.5 A0 A0 B9.5 B8.5 B8.5 B7
N tot 7763 6061 4998 12957 9781 8101 6756 5943 4998 11524 9622 8101
N(MVlim) 2209 1565 672 1587 935 278 821 653 361 446 289 133
N (1.2–3 kpc) 851 733 349 403 326 106 441 378 185 151 111 33
N / N S1 1.00 0.86 0.65 1.00 0.81 0.63 1.00 0.86 0.82 1.00 0.74 0.57

Notes. Spectral type according to the MVlim are shown. N is the number of stars for the absolute magnitude limited samples, i.e., MVlim(1.2 kpc)<MV<MVlim(3 kpc), also indicating which of them are between 1.2 and 3 kpc. N/NS1 is the ratio between the number stars (between 1.2 and 3 kpc) of each sample and the S1 sample, always using the MV range of the sample.

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