Table 1
Number of identified YSOs in each cluster, separated by identification method.
| Star cluster | Spectroscopic targets observed | |EW(Hα)| > 10 Å | EW(Li) > 0.15 Å | Spectroscopically flagged YSOs | Gaia variability YSOs (Marton et al. 2023) | Total YSOs |
|---|---|---|---|---|---|---|
| NGC 2264 N&S | 199 | 64 | 85 | 124 | 268 | 354 |
| Collinder 95 | 202 | 19 | 23 | 35 | 104 | 130 |
| Collinder 359 | 212 | 0 | 7 | 7 | 2 | 7 |
Notes. For YSOs identified by Gaia YSO variability (Marton et al. 2023), we only include stars with a G-band mean flux divided by its error greater than 50, an integrated RP mean flux divided by its error greater than 20, an integrated BP mean flux divided by its error greater than 20, and greater than 5 visibility periods.
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