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Table B.1

Excerpt of a few sources from our submillimetre catalogue.

ID Field RA Dec Global Source total fluxes N(H2)
signi- 160 μm 250 μm 350 μm 500 μm peak
[deg] [deg] ficance [Jy] [Jy] [Jy] [Jy] [cm-2]

3177 G70.10-1.69 303.68458 31.93218 2.1(2) 36.4 ± 0.9 27.5 ± 0.8 20.4 ± 0.5 8.7 ± 0.3 1.6 ± 0.1(22)
3178 G70.10-1.69 303.18555 31.66420 1.1(2) 13.1 ± 1.0 12.5 ± 0.6 9.8 ± 0.3 4.5 ± 0.1 8.9 ± 0.4(21)
3179 G70.10-1.69 303.64278 31.95605 1.2(2) 12.7 ± 1.1 17.0 ± 0.9 15.8 ± 0.7 9.5 ± 0.3 1.7 ± 0.1(22)
3180 G70.10-1.69 303.71176 32.01705 1.1(2) 7.5 ± 2.2 5.8 ± 1.1 4.0 ± 0.6 2.3 ± 0.3 8.7 ± 0.7(21)
3181 G70.10-1.69 303.29154 31.68988 1.1(2) 7.8 ± 0.6 18.9 ± 0.5 15.2 ± 0.3 8.2 ± 0.1 1.4 ± 0.0(22)
3182 G70.10-1.69 303.50257 32.01464 1.0(2) 17.6 ± 1.4 19.0 ± 1.2 12.7 ± 0.6 6.4 ± 0.2 1.1 ± 0.1(22)
3183 G70.10-1.69 303.61878 32.14447 9.7(1) 0.0 ± 0.0 14.8 ± 0.6 9.2 ± 0.3 4.0 ± 0.1 8.2 ± 0.2(21)
3184 G70.10-1.69 303.67175 32.15103 9.6(1) 0.0 ± 0.0 14.4 ± 0.7 6.9 ± 0.3 2.6 ± 0.1 5.2 ± 0.2(21)
3185 G70.10-1.69 303.47865 32.01340 8.7(1) 16.6 ± 1.9 19.1 ± 1.1 11.8 ± 0.6 5.7 ± 0.2 8.4 ± 0.5(21)
3186 G70.10-1.69 303.52968 31.64210 1.0(2) 24.6 ± 2.1 14.1 ± 0.7 14.4 ± 0.5 8.5 ± 0.2 1.6 ± 0.1(22)

3893 G300.869.00 186.12982 71.83428 1.0(2) 11.0 ± 0.6 17.7 ± 0.5 12.9 ± 0.4 5.8 ± 0.2 3.5 ± 0.3(21)
3894 G300.869.00 186.39477 71.70384 1.1(2) 41.5 ± 1.5 49.8 ± 0.8 35.6 ± 0.5 18.0 ± 0.2 4.5 ± 0.2(21)
3895 G300.869.00 186.11911 71.85208 7.1(1) 1.3 ± 0.3 3.1 ± 0.2 2.3 ± 0.2 1.1 ± 0.1 1.8 ± 0.3(21)
3896 G300.869.00 186.44020 71.65249 3.0(1) 1.3 ± 0.2 1.4 ± 0.1 0.9 ± 0.1 0.6 ± 0.0 8.2 ± 1.3(20)
3897 G300.869.00 186.07648 71.87277 2.8(1) 3.3 ± 0.4 4.9 ± 0.3 3.7 ± 0.2 1.7 ± 0.1 1.7 ± 0.3(21)
3898 G300.869.00 185.96055 71.90514 3.2(1) 0.0 ± 0.0 2.7 ± 0.2 1.9 ± 0.1 0.8 ± 0.1 7.4 ± 2.3(20)
3899 G300.869.00 186.25427 71.76398 2.6(1) 0.9 ± 0.5 1.1 ± 0.3 0.8 ± 0.2 0.3 ± 0.1 4.1 ± 1.9(20)
3900 G300.869.00 185.99452 71.85818 3.4(1) 3.3 ± 0.3 2.0 ± 0.3 1.9 ± 0.2 1.1 ± 0.1 1.5 ± 0.2(21)
3901 G300.869.00 185.86226 71.94612 2.4(1) 0.0 ± 0.0 1.6 ± 0.1 1.0 ± 0.1 0.5 ± 0.0 5.8 ± 0.8(20)
3902 G300.869.00 186.17681 71.68646 1.8(1) 0.7 ± 0.2 0.5 ± 0.1 0.3 ± 0.1 0.1 ± 0.0 2.6 ± 1.0(20)
ID FWHM Position angle SED fit Evolution
major minor east from north F(200 μm) T dust N(H2) M stage
[′′] [′′] [deg] [Jy] [K] [cm-2] [M]

3177 60.1 40.8 174.1 28.07 12.9 3.7(22) 1.4(2) PS1a
3178 56.3 40.4 105.6 12.15 12.3 2.3(22) 8.0(1) ?
3179 80.5 48.5 77.8 12.49 10.2 4.7(22) 2.7(2) ?
3180 57.6 40.0 11.1 4.76 11.5 1.3(22) 4.6(1) PS2
3181 69.5 45.1 30.4 15.85 11.2 3.8(22) 1.8(2) PS1b
3182 67.7 43.7 44.5 17.80 12.5 2.3(22) 1.0(2) PS1b
3183 59.9 40.0 163.5 16.27 14.2 1.3(22) 4.9(1) PS2
3184 44.5 40.0 176.3 19.43 18.3 6.8(21) 1.8(1) PS1b
3185 64.1 43.1 51.6 19.24 13.4 1.9(22) 7.8(1) PS1b
3186 63.4 56.6 2.8 10.29 10.0 4.9(22) 2.6(2) PS1b

3893 137.8 68.3 8.4 17.58 12.7 6.6(21) 4.8(1) ?
3894 179.4 134.5 8.4 45.80 12.2 8.7(21) 1.6(0) ?
3895 74.4 42.5 91.9 2.88 12.2 4.2(21) 1.0(1) SL1b
3896 74.4 49.8 111.0 1.12 11.4 2.0(21) 5.8(2) ?
3897 74.6 70.1 118.8 4.64 12.3 3.9(21) 1.6(1) ?
3898 71.4 66.7 174.3 2.67 12.9 1.8(21) 6.7(2) ?
3899 70.2 40.0 61.0 1.13 13.1 1.2(21) 2.6(2) SL1b
3900 82.6 56.8 54.3 1.50 10.3 4.3(21) 1.6(1) ?
3901 65.8 62.3 120.2 1.75 14.1 8.7(20) 2.8(2) ?
3902 75.0 40.0 129.3 0.58 14.0 4.0(20) 9.4(3) ?

Notes. The columns of the upper table give (1) the source ID number in our catalogue; (2) the field where the source was observed; (3) the source right ascension; (4) the source declination; (5) the source global significance from getsources; (6)(9) the source total fluxes from getsources from 160 to 500 μm with the corresponding uncertainties; (10) the source peak column density from getsources with the corresponding uncertainty. The columns of the lower table give: (1) the source ID number in our catalogue; (2) and (3) the source major and minor FWHM from getsources; (4) the source position angle from getsources; (5)(8) flux at 200 μm, dust temperature, column density, and mass of the source, all four derived from the SED fitting of the fluxes given in Cols. (6)(10) of the upper table; (9) stage of evolution of the source (PS1a: protostellar according to submillimetre data analysis, PS1b: protostellar according to mid-IR data analysis, PS2: according to both methods, SL1a: starless according to submillimetre data analysis, SL1b: starless according to mid-IR data analysis, SL2: according to both methods, ?: undetermined). The numbers in parentheses are powers of ten (e.g. 1.5(4) = 1.5 × 104).

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