Table 1
Summary of recent studies on clump fragmentation carried out on interferometric data of continuum emission.
| Survey Name | # Targets | Facility | Wavelengtha (mm) | Best angular resolution (″) | Reference |
|---|---|---|---|---|---|
| − | 4 | PdBI | 1.3 | 0.4 | Palau et al. (2013) |
| CORE | 20 | NOEMA | 1.3 | 0.4 | Beuther et al. (2018a) |
| ASHES | 39 | ALMA | 1.3 | 1.2 | Sanhueza et al. (2019); Morii et al. (2023) |
| − | 12 | ALMA | 1.3 | 0.8 | Svoboda et al. (2019) |
| ATOMS | 146 | ALMA | 3 | 1.2 | Liu et al. (2020) |
| − | 6 | ALMA | 3 | 2.8 | Anderson et al. (2021) |
| ALMA-IMF | 59 | ALMA | 1.3; 3 | 0.3 | Motte et al. (2022) |
| SQUALO | 13 | ALMA | 1.3; 3 | 1.1 | Traficante et al. (2023) |
| TEMPO | 38 | ALMA | 1.3 | 0.8 | Avison et al. (2023) |
| − | 59 | ALMA | 1.3 | 1 | Olmi et al. (2023) |
| QUARKS | 139 | ALMA | 1.3 | 0.25 | Liu et al. (2024); Xu et al. (2024b) |
| ASSEMBLE | 11 | ALMA | 0.87 | 0.8 | Xu et al. (2024a) |
| − | 16 | SMA | 0.87 | 0.6 | Pandian et al. (2024) |
| − | 13 | NOEMA, ALMA | 3 | 5.5 | Rigby et al. (2024) |
| INFANT | 8 | ALMA | 1.3 | 0.6 | Cheng et al. (2024) |
| DIHCA | 30 | ALMA | 1.3 | 0.06 | Ishihara et al. (2024) |
| ALMAGAL | 1013 | ALMA | 1.3 | 0.15–0.3b | Molinari et al. (2025) |
Notes. (a)The quoted wavelength is only indicative (e.g., 1.3 and 3 mm generically indicate ALMA Band 6 and 3, respectively); its precise value varies from case to case depending on the adopted spectral window(s).(b)The double value arises from the use of two interferometer configurations in ALMAGAL.
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