Table 4
HD 181327 photometric observations from the literature.
| Wavelength | Flux | Uncertainty | Instrument |
| (μm) | (Jy) | (Jy) | & Reference |
|
|
|||
| 12 | 0.114 | 0.011 | IRAS [1] |
| 15.0 | 0.094 | 0.004 | Spitzer/IRS [2] |
| 16.3 | 0.097 | 0.005 | Spitzer/IRS [2] |
| 17.4 | 0.107 | 0.005 | Spitzer/IRS [2] |
| 18.3 | 0.114 | 0.003 | T-ReCS [3] |
| 18.7 | 0.125 | 0.007 | Spitzer/IRS [2] |
| 19.8 | 0.144 | 0.009 | Spitzer/IRS [2] |
| 20.4 | 0.149 | 0.008 | Spitzer/IRS [2] |
| 21.1 | 0.157 | 0.020 | Spitzer/IRS [2] |
| 23.1 | 0.224 | 0.007 | Spitzer/IRS [2] |
| 23.7 | 0.223 | 0.009 | Spitzer/MIPS [1] |
| 25 | 0.306 | 0.024 | IRAS [1] |
| 25.7 | 0.303 | 0.014 | Spitzer/IRS [2] |
| 28.0 | 0.384 | 0.014 | Spitzer/IRS [2] |
| 30.6 | 0.488 | 0.026 | Spitzer/IRS [2] |
| 33.1 | 0.623 | 0.025 | Spitzer/IRS [2] |
| 35.5 | 0.718 | 0.034 | Spitzer/IRS [2] |
| 54.5 | 1.88 | 0.09 | MIPS-SED [4] |
| 58.0 | 1.83 | 0.07 | MIPS-SED [4] |
| 60 | 1.73 | 0.17 | ISO [5] |
| 61.4 | 1.98 | 0.08 | MIPS-SED [4] |
| 64.9 | 2.01 | 0.08 | MIPS-SED [4] |
| 68.4 | 1.98 | 0.08 | MIPS-SED [4] |
| 71.4 | 1.73 | 0.12 | Spitzer/MIPS [1] |
| 71.6 | 1.99 | 0.09 | MIPS-SED [4] |
| 75.1 | 1.93 | 0.10 | MIPS-SED [4] |
| 78.4 | 1.81 | 0.10 | MIPS-SED [4] |
| 81.8 | 1.72 | 0.11 | MIPS-SED [4] |
| 85.3 | 1.62 | 0.11 | MIPS-SED [4] |
| 88.8 | 1.47 | 0.11 | MIPS-SED [4] |
| 90 | 1.41 | 0.14 | ISO [5] |
| 92.0 | 1.46 | 0.13 | MIPS-SED [4] |
| 95.5 | 1.37 | 0.17 | MIPS-SED [4] |
| 100 | 1.7 | 0.2 | IRAS [1] |
| 155.9 | 0.77 | 0.09 | Spitzer/MIPS[1] |
| 170 | 0.736 | 0.192 | ISO [5] |
| 870 | 0.052 | 0.006 | LABOCA [6] |
| 3190 | 7.2 × 10-4 | 2.5 × 10-4 | ATCA [7] |
Notes. The Herschel continuum values used for the dust modeling are in Tables 2 and 3. All uncertainties are 1σ and include absolute calibration error.
References. [1] Schneider et al. (2006), [2] this study, data reduced with the Spitzer/c2d team pipeline (Lahuis et al. 2006), [3] Gemini, Chen et al. (2008), [4] Spitzer, Chen et al. (2006), [5] Moór et al. (2006), [6] APEX, Nilsson et al. (2009), [7] this study, Sect. 2.2.
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