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Table 3.
Source apertures and sky background annuli used to obtain PACS source photometry.
| Name | Band | Source | Sky (Rinner, Router) |
|---|---|---|---|
| annulus | annulus | ||
| (″) | (″, ″) | ||
| Recommended | Blue | 12 | (35, 45) |
| Green | 12 | (35, 45) | |
| Red | 22 | (35, 45) | |
| OH 21.5 +0.5 | Blue | 40 | (40, 60) |
| Red | 15 | (40, 60) | |
| OH 30.1 −0.7 | Blue | 40 | (40, 60) |
| Red | 25 | (40, 60) | |
| IRAS 18488−0107 | Blue | 40 | (40, 60) |
| Red | 15 | (40, 60) | |
| OH 32.8 −0.3 | Blue | 25 | (25, 30) |
| Red | 25 | (25, 40) | |
| IRAS 19067+0811 | Blue | 30 | (40, 60) |
| Red | 10 | (20, 25) |
Notes. Source apertures and sky background annuli used for the HIPE annularSkyAperturePhotometry task to obtain PACS source photometry. The recommended apertures are adopted for all sources, except for the ones that are explicitly listed.
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