Open Access
Table 2
Summary of Herschel and ancillary infrared/sub-mm photometry used in disc SED fitting.
| Wavelength | Fobs | Instrument |
| [μm] | [mJy] | |
|
|
||
| 9 | 1237 ± 17 | AKARI/IRC PSC, Ishihara et al. (2010) |
| 18 | 263 ± 31 | AKARI/IRC PSC, Ishihara et al. (2010) |
| 24 | 155 ± 5.3 | Spitzer/MIPS, Trilling et al. (2008). |
| 32 | 111 ± 5.1 | Spitzer/IRS |
| 70 | 278 ± 11 | Spitzer/MIPS, Trilling et al. (2008) |
| 160 | 250 ± 40 | Spitzer/MIPS, Krist et al. (2010) |
| 160 | 158 ± 20 | Spitzer/MIPS, Tanner et al. (2009) |
| 70 | 284 ± 1.5 | Herschel/PACS |
| 100 | 311 ± 1.1 | Herschel/PACS |
| 160 | 211 ± 1.5 | Herschel/PACS |
| 250 | 113 ± 18 | Herschel/SPIRE |
| 350 | 44.3 ± 9 | Herschel/SPIRE |
| 500 | 25.9 ± 8 | Herschel/SPIRE |
| 870 | 5 ± 3 | APEX/LABOCA, Nilsson et al. (2010) |
Notes. Uncertainties 1-σ and driven by the sky noise. Herschel calibration uncertainties are 10% for PACS and 15% for SPIRE.
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