Table 1
Colour-corrected photometry of AU Mic.
| Wavelength | Flux density | Telescope/ | Ref. | Ref. |
| [μm] | [mJy] | Instrument | Flux | Col. corr. |
|
|
||||
| 3.35 | 4820 ± 119 | WISE | C12, W10 | W10 |
| 4.6 | 4260 ± 119 | WISE | C12, W10 | W10 |
| 5.8 | 2200 ± 55 | Spitzer/IRAC | C05 | IH |
| 8 | 1270 ± 20 | Spitzer/IRAC | C05 | IH |
| 9 | 912 ± 22 | Akari | I10 | IH |
| 11.6 | 543 ± 60 | WISE | C12 | W10 |
| 12 | 517 ± 30 | IRAS | M90 | B88 |
| 18 | 246 ± 36 | Akari | I10 | IH |
| 22.1 | 183 ± 21 | WISE | C12 | W10 |
| 24 | 158 ± 3 | Spitzer/MIPS | P09 | IH |
| 25 | 244 ± 63 | IRAS | M90 | B88 |
| 60 | 269 ± 46 | IRAS | M90 | B88 |
| 70 | 227 ± 27 | Spitzer/MIPS | P09 | IH |
| 70 | 231 ± 16 | Herschel/PACS | HSA | IH |
| 100 | 680 ± 149 | IRAS | M90 | B88 |
| 160 | 172 ± 21 | Spitzer/MIPS | R08 | IH |
| 160 | 243 ± 17 | Herschel/PACS | HSA | IH |
| 250 | 134 ± 8 | Herschel/SPIRE | HSA | IH |
| 350 | 72 ± 21 | CSO/SHARCII | C05 | ... |
| 350 | 84.4 ± 5.4 | Herschel/SPIRE | HSA | IH |
| 450 | 85 ± 42 | JCMT/SCUBA | L04 | ... |
| 500 | 47.6 ± 3.8 | Herschel/SPIRE | HSA | IH |
| 850 | 14.4 ± 1.8 | JCMT/SCUBA | L04 | ... |
| 1300 | 8.5 ± 2.0 | SMA | W12 | ... |
| 1300 | 8.75 ± 0.98 | ALMA | M13 | ... |
Reference. B88: Beichman et al. (1988); C05: Chen et al. (2005); C12: Cutri & et al. (2012); HSA: Herschel Science Archive (Matthews et al., in prep.). IH: corresponding instrument hand book. I10: Ishihara et al. (2010); L04: Liu et al. (2004); M90: Moshir et al. (1990); M13: MacGregor et al. (2013); P09: Plavchan et al. (2009); R08: Rebull et al. (2008); W10: Wright et al. (2010); W12: Wilner et al. (2012). The ALMA and Herschel data were re-analysed in the present work.
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