Table 2.
Summary of the considered model variants, the adopted SFH, extinction map, data used for the fitting and Poissonian distance (δP).
| Model | SFH | Extinction | Fitted to | δP |
|---|---|---|---|---|
| MP-S | Exponential | Stilism | Tycho-2 V < 11 | 7.5 × 105 |
| G12Exp-S | Exponential | Stilism | Gaia DR2 G < 12 | 7.4 × 105 |
| G12NP-S | Non-param. | Stilism | Gaia DR2 G < 12 | 5.6 × 105 |
| G12NP-D | Non-param. | Drimmel | Gaia DR2 G < 12 | 5.4 × 105 |
| G12NP-M | Non-param. | Marshall | Gaia DR2 G < 12 | 6.0 × 105 |
Notes. The G12NP-S is our fiducial case. The MP-S model was derived in Mor et al. (2018; see their Fig. 7), its slopes of the IMF are α1 = 0.5, α2 = 2.1 and α3 = 2.9. The extinction maps named Stilism, Drimmel, and Marshall are from Lallement et al. (2018), Drimmel & Spergel (2001), and Marshall et al. (2006), respectively.
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