Table 3
Fit coefficients for the Galaxy seen through the far sidelobes.
| Frequency | Primary spillover | Secondary spillover | ||||
|
|
|
|||||
| [GHz] | fit | predictiona | direct | baffle | predictionb | |
|
|
||||||
| 100 ........... | −25.8 ± 5.7 | 7 | 26.3 ± 15.7 | 56.7 ± 5.7 | 10 | |
| 143 ........... | −9.1 ± 4.1 | 6 | 13.0 ± 4.8 | 23.8 ± 5.4 | 10 | |
| 217 ........... | 0.6 ± 1.1 | 5 | 6.3 ± 2.1 | 6.5 ± 1.3 | 6 | |
| 353 ........... | −1.2 ± 0.5 | 1 | −4.3 ± 2.1 | 3.6 ± 0.7 | 1 | |
| 545 ........... | 7.7 ± 1.7 | 15 | 8.8 ± 3.1 | 7.9 ± 1.0 | 1 | |
| 857 ........... | 17.1 ± 3.4 | 1.5 | 23.9 ± 4.2 | 16.7 ± 3.1 | 0.005 | |
Notes.
Unitless value we would expect for the fit to the primary spillover sidelobe contribution. It is the ratio of the primary spillover at the given frequency to the spillover at 353 GHz, as calculated in Table 2 of Tauber et al. (2010). If all our data and predictions were perfect, this value would match the corresponding value in the column labelled “Fit”.
Unitless value we would expect for the fit to the secondary spillover sidelobe contribution. It is the ratio of the secondary spillover at the given frequency to the spillover at 353 GHz, as calculated in Table 2 of Tauber et al. (2010). If all our data and predictions were perfect, this value would match the corresponding fit values in the columns labelled “Direct” and “Baffle”, which would also be equal to each other.
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