Table 2.
Selected parameters for the DCEPs sample.
| Source_id | ℓ | b | d | μ | σμ | [Fe/H] | σ[Fe/H] | Flag | Source | logAge | σlogAge |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | (kpc) | (mag) | (mag) | (dex) | (dex) | (dex) | (dex) | |||
| 4060910068247394432 | 0.38444 | 1.96190 | 8.02 | 14.522 | 0.129 | 0.50 | 0.20 | 1 | P21 | 8.594 | 0.016 |
| 4049125051634137600 | 0.45968 | −5.42326 | 14.46 | 15.801 | 0.117 | 0.19 | 0.20 | 1 | P21 | 8.706 | 0.015 |
| 4048895253682114432 | 0.47058 | −6.65562 | 19.14 | 16.410 | 0.114 | −0.05 | 0.20 | 1 | Gaia_DR3 | 8.623 | 0.015 |
| 4056461478623363968 | 359.98638 | −1.45395 | 15.81 | 15.995 | 0.157 | 0.11 | 0.20 | 1 | Gaia_DR3 | 7.715 | 0.015 |
Notes. The full table is available at the CDS. The source_id is the Gaia source_id, ℓ and b are the galactic coordinates; d is the heliocentric distance in kpc; μ and σμ are the distance modulus and its uncertainty; [Fe/H] and σ[Fe/H] are the iron abundance and its uncertainty; flag = 0 or 1 means that the metallicity was taken from the astrophysical parameters or calculated from the metallicity gradient of the Galactic disc; source lists the provenance of the DCEP source: Gaia_DR3 means that the star is included in the Gaia DR3 vari_cepheids catalogue, P21 or Inno indicate that the DCEPs were taken from the Pietrukowicz et al. (2021) or Inno et al. (2021) catalogues, respectively; logAge and σlogAge are the decimal logarithm of the age and its uncertainty.
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