Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/202245399e]


Table 1.

Summary of the datasets for which we deliver StarHorse parameters in this work.

Survey
LAMOST DR7 LRS 6 179 327 4 803 496 4 531 028 1 206 381 131 845
LAMOST DR7 MRS 738 025 457 359 425 281 106 125 15 547
SDSS DR12 (optical) 503 967 258 194 249 991 68 391 13 584
GALAH DR3 588 571 581 149 557 559 127 016 26 318
RAVE DR6 517 095 515 800 471 490 94 765 23 809
APOGEE DR17 733 901 720 970 562 424 61 331 15 060
GES DR5 114 324 75 008 67 562 11 542 3320
Gaia DR3 RVS 5 594 205 4 833 548 4 211 087 799 149 178 719

Survey Model resolution Bestfilter Parallaxes
LAMOST DR7 LRS agestep = 0.1; metstep = 0.05 Ks2MASS 99%
LAMOST DR7 MRS agestep = 0.05; metstep = 0.02 Ks2MASS 77%
SDSS DR12 (optical) agestep = 0.1; metstep = 0.05 parallax 100%
GALAH+DR3 agestep = 0.05; metstep = 0.02 Ks2MASS 98%
RAVE DR6 agestep = 0.1; metstep = 0.05 Ks2MASS 86%
APOGEE DR17 agestep = 0.05; metstep = 0.02 H2MASS 75%
GES DR5 agestep = 0.05; metstep = 0.02 H2MASS 97%
Gaia DR3 RVS agestep = 0.1; metstep = 0.05 GGaia 100%

Notes. Upper rows show the main numbers of input catalogue sources, those that survived the quality cuts, those for which the code converged to a solution, and the number of MSTO and subgiants selected on the output. The lower rows show the model configuration and parallax coverage for the final input catalogues.

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