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Table D.2.

Evolutionary state classification of the submillimetre compact sources.

ID Type N(H2) Td ΔTd w1 − w2 w3 − w4 Type Gaia match π Comment
(cm−2) (K) (K) (mas)
1446 4 4.4(22) 17.1 4.2 ± 0.8 cp cp 0/I Outflows, HH objects
1447 4 8.7(22) 13.1 −1.3 ± 0.9 cp cp 0/I Several YSOs, outflows, HH objects
1448 4 3.8(22) 14.1 −0.2 ± 0.9 cp cp 0/I Source detected at 3−500 μm
1449 4 5.0(22) 10.2 −2.1 ± 0.3 cp cp 0/I Source detected at 3−500 μm
1450 0 7.9(22) 9.9 −2.0 ± 0.4 cp bg III/F 3351030967214777984 1.45 ± 0.05 100 μm emission : Possibly one Class 0 YSO
1451 3 2.9(22) 12.7 −0.8 ± 0.4 cp cp III/F Source detected at 3−500 μm ≠ Rapson
1452 4 2.7(22) 13.0 −0.9 ± 0.4 cp cp II 3350981656693549696 1.76 ± 0.36 Source detected at 3−500 μm
1453 2 4.5(22) 9.4 −2.6 ± 0.4 bg bg AGN Large spatial shift
1454 4 5.2(22) 9.8 −2.2 ± 0.4 cp cp 0/I Source detected at 3−500 μm – Several YSOs
1455 0 2.9(22) 10.1 −1.9 ± 0.3 cp bg III/F 3326958152260041600 1.7 ± 0.2 NIR source is CIII/F, but compact source at 100 μm
1456 1 2.4(22) 12.2 −1.9 ± 0.2 cp bg III/F
1457 4 2.0(22) 11.7 −0.7 ± 0.2 cp cp 0/I Detected at 3−500 μm – Substructured, at least one YSO
1458 2 1.4(22) 11.4 −1.2 ± 0.3 bg
1459 1 9.6(21) 12.2 −0.8 ± 0.3 bg bg III/F 3350983683919806848 3.29 ± 0.87 2MASS = Gaia ≠ Rapson
1460 2 1.9(22) 11.1 −1.3 ± 0.3 cp III/F 3351030417458975616 1.98 ± 0.03
1461 2 1.6(22) 11.7 −1.2 ± 0.4
1462 2 1.1(22) 11.0 −1.0 ± 0.4 bg
1463 2 1.1(22) 11.4 −0.9 ± 0.2
1464 1 6.2(21) 11.9 −0.6 ± 0.1 cp bg III/F 3351033883496495744 1.45 ± 0.14 2MASS = Gaia ≠ Rapson
1465 2 1.1(22) 11.7 −1.5 ± 0.3 bg
1466 1 6.3(21) 13.9 −0.6 ± 0.2 cp bg 3350978602973521280 3.4 ± 0.7
1467 0 1.5(22) 11.9 −1.0 ± 0.3 cp bg III/F Several unclassified NIR/MIR point sources
1468 3 7.5(21) 13.7 −0.3 ± 0.3 cp cp III/F 3351046394737185408 1.29 ± 0.05 Source detected at 3−500 μm – real CIII?
1469 2 2.1(22) 9.4 −1.8 ± 0.2 cp bg III/F 3351056973241029248 1.9 ± 0.04
1470 1 5.8(21) 13.5 −0.7 ± 0.2 bg bg
1471 4 6.3(21) 12.3 −0.8 ± 0.2 cp cp 0/I Several foreground/background sources, one real YSO
1472 1 1.7(22) 8.8 −0.6 ± 0.2 cp+bg bg III/F
1473 2 6.3(21) 12.0 −1.2 ± 0.2 bg
1474 2 1.3(22) 12.0 −0.6 ± 0.4 bg
1475 2 4.4(21) 12.7 −0.6 ± 0.2 cp III/F 3326959011253582848 1.2 ± 0.7 Large spatial shift
1476 2 1.4(22) 9.9 −0.3 ± 0.3 cp III/F Large spatial shift
1477 2 2.7(21) 14.0 −0.7 ± 0.8 cp bg III/F
1478 2 6.3(21) 12.2 −0.7 ± 0.4 cp III/F 3351040858523618816 1.19 ± 0.24 Gaia = Rapson, large spatial fit
3351040858524306944 1.26 ± 0.37 Gaia = 2MASS, large spatial fit
1479 2 6.3(21) 12.7 −1.0 ± 0.2 cp Large spatial shift
1480 2 7.3(21) 11.9 −0.9 ± 0.3 cp III/F 3351030795416094848 1.76 ± 0.11
1481 3 4.7(21) 13.7 −0.7 ± 0.2 cp cp II 3326961794392311424 1.62 ± 0.39 Missing compact emission at 100 μm
1482 2 7.5(21) 11.4 −0.9 ± 0.4 cp III/F 3350981862852157056 0.36 ± 0.29 Large spatial shift
1483 2 5.7(21) 10.4 −1.4 ± 0.2 cp III/F 3351032101084459776 0.6 ± 1 Large spatial shift
1484 0 5.1(21) 12.6 −0.4 ± 0.1 cp III/F 335105645784390912 −1.6 ± 0.8 Type = CIII/F, but compact emission at 100μm
1485 2 1.3(22) 10.1 −1.9 ± 0.3 cp bg III/F 3351089000812448640 1.69 ± 0.09 2MASS = Rapson ≠ Gaia
1486 2 2.2(21) 18.2 0.3 ± 0.4 cp cp III/F 3350983069739510528 0.2 ± 0.8
1487 1 2.6(21) 13.9 −1.1 ± 0.1 cp+bg bg
1488 2 3.1(21) 12.7 −0.3 ± 0.1 bg
1489 2 2.9(21) 15.3 0.6 ± 0.2 cp bg III/F Probable warm starless core
1490 0 3.0(21) 14.4 −0.8 ± 0.2 cp bg 3327782889059332480 1.37 ± 0.2 Good spatial and distance match, but no MIR detection
1491 2 3.8(21) 15.1 −0.1 ± 0.1 cp bg III/F 3351038453342829952 Large spatial shift
1492 1 5.9(21) 10.8 −0.8 ± 0.2 cp bg III/F 3351043710382744832 Substructured
1493 2 1.1(22) 10.1 −1.0 ± 0.2 bg bg
1494 0 1.5(21) 14.8 −0.5 ± 0.2 cp cp 3327031995634205952 0.27 ± 0.05 2MASS = Gaia (background), but 100 μm emission
1495 2 2.6(21) 13.2 0.1 ± 0.2 cp bg III/F Core-shaped emission at 100 μm
1496 1 3.4(21) 11.5 −0.5 ± 0.2 cp bg PAH
1497 3 8.0(20) 15.9 0.1 ± 0.4 cp cp 0/I YSO candidate not detected at 100 μm
1498 2 3.0(21) 15.0 −0.3 ± 0.2 cp bg III/F 3351057522995678208 0.35 ± 0.22
1499 2 2.4(21) 14.7 0.5 ± 0.1 cp core III/F 3351061955401965952 1.1 ± 0.1 Warm starless – Core-shaped emission at 12−160 μm
1500 1 3.4(21) 11.3 −0.9 ± 0.2 cp III/F
1501 1 3.2(21) 15.0 0.1 ± 0.2 cp III/F
1502 2 3.7(21) 11.3 −0.5 ± 0.3 cp III/F 3351040514926184960 0.21 ± 0.15
1503 2 3.5(21) 11.9 −0.2 ± 0.1 bg bg
1504 2 2.0(21) 14.1 −0.2 ± 0.1 cp bg 3350978564318784896 4.6 ± 0.6
1505 0 4.9(21) 13.0 −0.3 ± 0.2 cp bg III/F 3326946233727400704 2 ± 0.2 2MASS = Rapson = Gaia, foreground
3326946233727399680 1.27 ± 0.26 Second Gaia source close to core peak
1506 2 2.4(21) 13.7 −0.5 ± 0.1 cp bg III/F 3351051475681700864 −0.1 ± 0.3
1507 1 4.2(21) 15.1 −0.4 ± 0.2 cp bg III/F 3351045604463218304 1.9 ± 0.2
1508 2 4.8(21) 12.4 −0.2 ± 0.1 bg bg
1509 9 8.4(20) 15.8 −0.1 ± 0.2 cp cp Galaxy: SED peak at 50 μm, very isolated from filament
1510 2 4.1(21) 11.4 −0.4 ± 0.1 cp 3326944648882916352 1.7 ± 0.6 Large spatial shift
1511 2 1.7(21) 16.8 −0.6 ± 0.2 cp cp 3351857387641672064 3.7 ± 1.3 The foreground point source is still visible at 22 μm
1512 2 4.2(21) 13.0 −0.3 ± 0.3
1513 2 1.2(21) 17.8 0.2 ± 0.1 cp core III/F 3350984268035096704 0.3 ± 0.3 Warm starless – Core-shaped emission at 12−160 μm
cp 3350984925165355904 1.33 ± 0.03 Large spatial shift
1514 2 2.6(21) 13.4 −0.3 ± 0.1 cp bg III/F 3351034089655997824 0.06 ± 0.55 2MASS = Rapson ≠ Gaia
1515 2 3.4(21) 11.2 −0.3 ± 0.1
1516 1 2.7(21) 12.4 −0.1 ± 0.3 cp bg Bright ridge emission at 12−100 μm
1517 2 2.7(21) 11.5 −0.4 ± 0.2 cp cp+bg III/F 3351035360964589440 −0.7 ± 0.9
1518 2 3.5(21) 13.4 −0.1 ± 0.3 cp III/F 3351039965171558912 Large spatial shift
1519 2 1.4(21) 16.7 0.3 ± 0.1 cp edge III/F 3351057458573023104 −0.8 ± 0.5 Warm starless – Core-shaped emission at 12−160 μm
1520 1 4.0(21) 12.0 −0.9 ± 0.1 cp III/F
1521 2 2.2(21) 13.7 −0.1 ± 0.1 cp cp III/F 3351056492203698304 3.15 ± 0.05
1522 1 3.4(21) 11.4 −0.3 ± 0.1 cp bg III/F 3351084632831098240 0.16 ± 0.49
1523 2 1.2(21) 13.2 0.2 ± 0.1 cp bg III/F 3350982137731278720 0.51 ± 0.27
1524 2 3.2(21) 11.6 −0.2 ± 0.0 cp bg III/F Large spatial shift
1525 2 3.0(21) 11.9 0.1 ± 0.2 mcp bg III/F
1526 2 1.9(21) 15.2 0.3 ± 0.1 mcp edge PAH Warm starless – Core-edge shaped emission at 12−100 μm
1527 2 2.8(21) 12.7 −0.7 ± 0.1 cp cp III/F 3351063574606062976 0.84 ± 0.11
1528 2 1.1(21) 14.3 0.2 ± 0.2 cp bg 3351056664002342784 0.48 ± 0.66 Warm starless – Core shaped emission at 100 μm
1529 2 1.2(21) 13.4 −0.2 ± 0.1 cp bg III/F 3351037942239970304 0.6 ± 0.5 2MASS ≠ Rapson = Gaia ; large shifts
1530 1 3.3(21) 13.7 −0.5 ± 0.2 mcp bg AGN
1531 1 1.2(21) 14.9 0.5 ± 0.1 cp+bg edge Warm starless – Core shaped emission at 12−22 μm
1532 1 1.8(21) 14.4 −0.4 ± 0.1 cp
1533 2 2.3(21) 13.2 −0.6 ± 0.1 mcp bg III/F 2MASS ≠ Rapson ; large shift for Rapson
1534 2 1.2(21) 16.2 0.2 ± 0.1 cp+bg core 3327028349205172736 0.3 ± 0.5 Warm starless – Core shaped emission at 12−100 μm
1535 2 2.1(21) 13.5 −0.2 ± 0.1 cp cp III/F 3326956885246723328 0.7 ± 0.3
1536 2 1.3(21) 14.5 −0.3 ± 0.2 mcp bg AGN 3351057973968718592 2.1 ± 0.6 2MASS = Gaia ≠ Rapson
1537 2 1.3(21) 13.3 −0.2 ± 0.1 cp cp III/F 3351090645784954624 0.21 ± 0.05 Large spatial shift
1538 1 6.0(21) 9.6 −0.1 ± 0.1 cp edge AGN 3350964820423096704 0.3 ± 1.1 2MASS = Gaia ≠ Rapson
1539 2 9.1(20) 13.5 −0.1 ± 0.1 cp core III/F 3351036941512554752 0.6 ± 1.2 Core shaped emission at 12−100 μm
1540 2 5.2(20) 18.8 −0.1 ± 0.1 cp core III/F 3327010791379052800 0.5 ± 0.3 Large spatial shift
1541 1 9.2(20) 13.9 0.2 ± 0.1 cp bg Warm starless – Core shaped emission at 100 μm
1542 1 1.2(21) 15.1 0.1 ± 0.1 mcp env. 3350964000083713664 0.5 ± 1 Envelope emission at 12 μm
1543 2 1.3(21) 14.6 −0.1 ± 0.1 mcp bg III/F 2MASS ≠ Rapson; large shifts

Notes. The columns are (1) the index of the source in the GCC catalogue; (2) new estimate of the evolutionary stage of the source. The code is 0 = undetermined, 1 = candidate starless core, 2 = confirmed starless core, 3 = candidate protostellar core, 4 = confirmed protostellar core. (3−4) Column density and dust temperature from the GCC catalogue; (5) variation (centre-background) in dust temperature and its uncertainty; (6) morphology type in the WISE 3.4 and 4.6 μm bands; cp means compact, mcp means that multiple compact sources are detected, bg means background, (7) morphology type in the WISE 12 and 22 μm bands; core means that the emission has the same morphology as the core at 250 μm; edge means that the emission corresponds to a bright edge of the core as seen at 250 μm; env. means envelope of the core seen at 250 μm; (8) type of the MIR source(s) as classified by Renaud et al. (2013); (9) identifier of Gaia source(s) that match the NIR or MIR source(s); (10) parallax of the Gaia sources.

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