Table 4
Description whether the fluxes measured in the on-source spaxel and the surrounding three by three spaxels are consistent with the pure spillover factor (0.70 at 79 μm, 0.69 at 84 μm, 0.62 at 119 μm, and 0.49 at 163 μm).
| Source | 79 μm | 84 μm | 119 μm | 163 μm | Spatially extended |
|
|
|||||
| NGC 1333 IRAS 2A | – | – | no (abs.) | – | – |
| NGC 1333 IRAS 4A | – | no | no | – | yes |
| NGC 1333 IRAS 4B | no | no | no | no | yes |
| L 1527 | no | yes | yes | yes | (no) |
| Ced110 IRS4 | yes | (yes) | yes | yes | no |
| IRAS 15398/B228 | no | no | no | no | yes |
| L 483 mm | (no) | yes | yes | – | (no) |
| Ser SMM1 | no | no | no | no | yes |
| Ser SMM3 | no | no | – | – | yes |
| L 723 mm | – | yes | yes | – | no |
|
|
|||||
| L 1489 | yes | yes | yes | yes | no |
| TMR 1 | no | no | no | yes | (mispointed) |
| TMC 1A | no | yes | – | yes | (no) |
| TMC 1 | no | no | – | yes | (yes) |
| HH 46 | no | yes | no | – | no |
| DK Cha | – | no | – | – | (yes) |
| RNO 91 | yes | – | – | – | no |
|
|
|||||
| AFGL 490 | no (abs.) | no (abs.) | no (abs.) | no | yes |
| NGC 2071 | no | no | no (abs./em.) | no | yes |
| NGC 7129 FIRS 2 | no | yes | no | – | yes |
| Vela IRS 17 | no | no | no (abs./em.) | no | yes |
| Vela IRS 19 | no | no | no (abs./em.) | no | yes |
| L1641 S3MMS1 | no | yes | no | yes | yes |
Notes. If the fraction of flux measured in the on-source spaxel compared to the three by three central spaxels is smaller than the spillover value, it is an indication that the OH line is spatially extended, as summarized in the last column.
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