Table 2
Nearby clouds considered for comparison with the CAFFEINE sample.
| Cloud | Dist kpc | RA ∘ | Dec ∘ | References(a) YSOs,  map |
|---|---|---|---|---|
| Aquila | 0.44 | 277.42 | −2.80 | 1, 4, 5, 6 |
| Ophiuchus | 0.13 | 246.88 | −24.21 | 1, 6, 7 |
| Orion B | 0.42 | 86.90 | 0.10 | 2, 6, 8 |
| Lupus I | 0.15 | 235.26 | −34.09 | 1, 6, 9 |
| Lupus III | 0.20 | 242.51 | −39.08 | 1, 6, 9 |
| Lupus IV | 0.15 | 241.15 | −42.07 | 1, 6, 9 |
| Corona Australis | 0.13 | 287.15 | −37.12 | 1, 6, 10 |
| Serpens | 0.48 | 278.75 | 0.00 | 1, 4, 6, 11 |
| Perseus | 0.25 | 53.92 | 31.53 | 1, 6, 12 |
| Chamaeleon I | 0.15 | 163.92 | −77.12 | 1, 6 |
| California | 0.47 | 65.00 | 37.69 | 3, 13 |
Notes. (a)References for the adopted distances, lists of YSOs and column density maps: (1) Dunham et al. (2015); (2) Megeath et al. (2012); (3) Lada et al. (2017); (4) Ortiz-León et al. (2023); (5) Könyves et al. (2015); (6) http://gouldbelt-herschel.cea.fr/archives (HGBS); (7) Ladjelate et al. (2020); (8) Könyves et al. (2020); (9) Benedettini et al. (2018); (10) Bresnahan et al. (2018); (11) Fiorellino et al. (2021); (12) Pezzuto et al. (2021); (13) (Zhang et al. 2024; Harvey et al. 2013).
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