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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