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Table 1.
Summary of data used in this paper.
| Band | Surveys | Spatial resolution | Sensitivity | Purpose | Ref. |
|---|---|---|---|---|---|
| NIR | UKIDSS-GPS | ∼1″ | K = 18.05 mag (5σ) | Identifying YSOs | Lucas et al. (2008) |
| NIR | VVV | ∼1″ | Ks ∼ 18 mag | Identifying YSOs | Minniti et al. (2010) |
| NIR | 2MASS | ∼4″ | Ks = 14.3 mag (10σ) | Identifying YSOs | Skrutskie et al. (2006) |
| MIR | GLIMPSE | ∼2″ | [8.0]=13.0 mag (3σ) | Identifying YSOs | Benjamin et al. (2003) |
| MIR | MIPSGAL | ∼6″ at 24 μm | ∼2 mJy at 24 μm | Identifying YSOs | Carey et al. (2009) |
| MIR | AllWISE | ∼6−12″ | Variablea | Identifying YSOs that are saturated on Spitzer images | Wright et al. (2010) |
| MIR | RMS | ∼18.3″ | ∼3 Jy at 21 μm (50% completeness)b | Including massive YSOs | Lumsden et al. (2013) |
| FIR | Hi-Gal | ∼6−35″ | ∼12.4 mJy at 70 μm (1σ) | Identifying protostellar objects | Molinari et al. (2010) |
| mm | GRS | 46″ | 0.27 K per 0.2 km s−1 (13CO) | Obtaining gas properties of GMFs | Jackson et al. (2006) |
| mm | ThrUMMS | 72″ | 0.7 K per 0.34 km s−1 (13CO) | Obtaining gas properties of GMFs | Barnes et al. (2015) |
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