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Table 2.
FIR and millimetric wavelength ≤1.5 mm surveys and their sensitivity at 5σ detection.
| Survey, instrument | Fields | Wavelenth (μm) | Minimum flux (5σ) (μJy) | Reference |
|---|---|---|---|---|
| Spitzer, MIPS | EGS, GOODS-N/-S, ECDFS | 70 | 2500–3500 | Magnelli et al. (2009) |
| Herschel/SPIRE, H-ATLAS | 500 sq. degrees | 250 | 25 500–60 000 | Eales et al. (2010) |
| Herschel/SPIRE, H-ATLAS | 500 sq. degrees | 350 | 28 000–60 500 | Eales et al. (2010) |
| Herschel/SPIRE, H-ATLAS | 500 sq. degrees | 500 | 33 000–65 000 | Eales et al. (2010) |
| Herschel/SPIRE, HerMES | Several | 250 | 3800–53 000 | Oliver et al. (2012) |
| Herschel/SPIRE, HerMES | Several | 350 | 3100–53 000 | Oliver et al. (2012) |
| Herschel/SPIRE, HerMES | Several | 500 | 4500–76 500 | Oliver et al. (2012) |
| Herschel/PACS, PEP | Several | 70 | 1700 | Lutz et al. (2011) |
| Herschel/PACS, PEP | Several | 100 | 900–7500 | Lutz et al. (2011) |
| Herschel/PACS, PEP | Several | 170 | 2200–16 400 | Lutz et al. (2011) |
| ALMA, ASPECS | HUDF | 1000 | 63.5 | Walter et al. (2016) |
| ALMA, ASPECS LP | HUDF | 1000 | 47.5 | Walter et al. (2016) |
| ALMA, GOODS | GOOD-S, 70 sq. arcmin. | 1100 | 900 | Franco et al. (2018) |
| ALMA, ASAGAO | GOOD-S, 26 sq. arcmin. | 1200 | 190 | Hatsukade et al. (2018) |
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