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Table 3.

Properties of SABOCA sources, their 24 μm and 70 μm associations, and parental clumps.

Name Distance M1σ Td N(H2) L1σ MIR type Parental clump
(kpc) (M) (K) (cm−2) (L)
GS301.1350−0.2220 4.6 208.0 31.1 1.56 × 1023 9.87 × 103 24sat G301.1365−0.2256
GS301.1364−0.2252 4.6 162.3 38.9 1.66 × 1023 2.40 × 104 22ct,70ct,24sat G301.1365−0.2256
GS301.1400−0.2233 4.6 217.2 29.1 1.05 × 1023 7.94 × 103 24sat G301.1438−0.2227
GS302.1493−0.9497 11.1 96.0 26.0 1.90 × 1022 2.23 × 103 22ct,70ct,24sat G302.1487−0.9494
GS303.1176−0.9717 1.6 1.9 30.1 1.92 × 1022 1.04 × 102 22ct,70ct,24sat G303.1169−0.9724
GS303.9991+0.2799 11.6 182.2 21.1 4.04 × 1022 1.23 × 103 22ct,70ct G303.9978+0.2804
GS304.7120+0.6001 2.3 5.2 15.5 3.07 × 1022 6.19 × 100 70ct G304.7127+0.6005
GS305.0947+0.2501 6.0 115.7 18.1 5.10 × 1022 3.17 × 102 70q G305.0943+0.2510
GS305.0997+0.2484 6.0 54.4 18.9 3.86 × 1022 1.95 × 102 70q
GS305.2566+0.3162 6.1 145.4 18.7 8.50 × 1022 4.70 × 102 70q

Notes. The columns are defined as follows: name: SABOCA catalog source name. Distance: distance of the source in kpc. M1σ: mass of the source by summing all the pixel values in the column density map according to Eq. (2), using a radius of 1σ. Td: average dust temperature of the source. N(H2): average column density of the source. Lsab: luminosity of the source by integrating the SED from 1 μm to 1 mm according to Eq. (3). MIR type: source mid-infrared association as described in Sect. 3.5. (24sat: associated with saturated 24 μm emission. 70ct: associated with PACS 70 μm compact source. 24ct: associated with MIPSGAL 24 μm compact source. 22ct: associated with WISE 22 μm compact source. HII: associated with (UC)HII regions. 70q: associated with extended 70 μm emission or 70 μm quiet). Parental clump: name of the ATLASGAL clump that the SABOCA core is associated with (Sect. 5.3). The full table is available at the CDS.

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