Table 3
Targets with possible contamination within the used apertures in MIPS24.
| Object | Fsource/Faper | N | Companion distance (′′) | Band | ||||||
|
|
||||||||||
| Sz651 | 0.4 | 1 | 6.5 | PACS70 | ||||||
| Sz661 | 2.9 | 1 | 6.2 | PACS70 | ||||||
| Sz1003 | 0.2 | 1 | 23.4 | SPIRE350 | ||||||
| Sz1032 | 0.8 | 10 | 41.2 | SPIRE500 | ||||||
| Sz1042 | 2.7 | 10 | 36.4 | SPIRE500 | ||||||
| Sz108B | 1.4 | 3 | 38.8 | SPIRE500 | ||||||
| 2MASSJ1608537* | 9.3 | 1 | 6.9 | PACS70 | ||||||
| Sz112 | 0.5 | 4 | 31.9 | SPIRE500 | ||||||
| SSTc2dJ161029.4-3922153 | 0.1 | 2 | 7.4 | PACS70 | ||||||
| SSTc2dJ160002.4-4222163 | 0.4 | 2 | 39.8 | SPIRE500 | ||||||
| SSTc2dJ160111.6-4137303 | 0.2 | 1 | 24.2 | SPIRE350 | ||||||
Notes. The second column shows the fraction of total MIPS24 flux in the aperture with that of the target.
The MIPS24 contamination affecting Sz65 is caused by Sz66, and vice versa, as can be seen in Fig. 4. This is taken into account in the photometry analysis.
The MIPS24 contamination affecting Sz103 is caused by Sz104, and vice versa, as can be seen in Fig. 4. This is taken into account in the photometry analysis.
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