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Table 2.

Characteristics of the synthetic diagrams used for the analysis of the GCNS SFH.

Synthetic mother color-magnitude diagrams

Name Age range [M/H] qmin β Library Mlim N* (×106) Shift
(Gyr) range (MG ≤ 5) (col, mag)
q01b03_60M_MG10 13.5–0.02 −2.2–0.45 0.1 0.3 BaSTI-IAC 10 7.0 (−0.036, 0.041)
q01b03_112M_MG6 13.5–0.08 −2.2–0.45 0.1 0.3 BaSTI-IAC 6 68.2 (−0.036, 0.040)
q01b03_120M_MG5 13.5–0.08 −2.2–0.45 0.1 0.3 BaSTI-IAC 5 120 (−0.035, 0.037)
q01b03_30M_MG10_parsec 13.5–0.02 −2.2–0.27 0.1 0.3 PARSEC 10 4 (−0.047,0.045)
q01b03_43M_MG5_parsec 13.5–0.02 −2.2–0.27 0.1 0.3 PARSEC 5 43.2 (−0.035,0.030)
q01b05_60M_MG10 13.5–0.02 −2.2–0.45 0.1 0.5 BaSTI-IAC 10 6.9 (−0.030, 0.030)
q01b07_30M_MG11 13.5–0.02 −2.2–0.45 0.1 0.7 BaSTI-IAC 11 2.2 (−0.027, 0.030)
q01b07_81M_MG5 13.5–0.02 −2.2–0.45 0.1 0.7 BaSTI-IAC 5 81.3 (−0.030, 0.030)
q04b03_30M_MG11 13.5–0.02 −2.2–0.45 0.4 0.3 BaSTI-IAC 11 2.2 (−0.034, 0.038)
q06b01_30M_MG10 13.5–0.02 −2.2–0.45 0.6 0.1 BaSTI-IAC 10 3.5 (−0.039, 0.048)

Notes. Columns, from left to right: identification name, which includes information on the millions (M) of stars down to a given limiting magnitude (MG); age and metallicity ranges; the minimum binary mass ratio (qmin); the binary fraction (β); the stellar evolution library; the limiting magnitude Mlim; the number of stars with a MG ≤ 5 mag; and the shift in colour and magnitude subtracted to the mother CMD.

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