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Table 4
Accuracy of AP estimation (internal rms errors) with the GSP-Phot algorithm Aeneas using BP/RP spectra and parallaxes, for stars covering the full AP space shown in Fig. 6.
| G | T eff | A 0 | log g | [Fe/H] | |
| mag | K | mag | dex | dex | |
|
|
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| A stars | 9 | 340 | 0.08 | 0.43 | 0.86 |
| 15 | 260 | 0.06 | 0.38 | 0.93 | |
| 19 | 400 | 0.15 | 0.51 | 0.74 | |
|
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| F stars | 9 | 150 | 0.06 | 0.36 | 0.36 |
| 15 | 170 | 0.07 | 0.38 | 0.33 | |
| 19 | 630 | 0.35 | 0.37 | 0.60 | |
|
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| G stars | 9 | 140 | 0.07 | 0.31 | 0.14 |
| 15 | 140 | 0.07 | 0.22 | 0.16 | |
| 19 | 450 | 0.33 | 0.45 | 0.65 | |
|
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| K stars | 9 | 100 | 0.09 | 0.26 | 0.19 |
| 15 | 90 | 0.08 | 0.26 | 0.21 | |
| 19 | 230 | 0.23 | 0.36 | 0.48 | |
|
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| M stars | 9 | 60 | 0.13 | 0.15 | 0.21 |
| 15 | 70 | 0.14 | 0.29 | 0.25 | |
| 19 | 90 | 0.13 | 0.17 | 0.29 | |
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