Open Access
Table 3
Properties of the beams used in this work.
| Band | Season | FWHM(′) | Solid Angle (10−9 sr) |
|---|---|---|---|
| f150 | 2008 | 1.367 | 216.3 ± 3.9 |
| 2009 | 1.375 | 216.2 ± 3.9 | |
| 2010 | 1.371 | 214.8 ± 3.9 | |
| f220 | 2008 | 0.997 | 116.6 ± 2.3 |
| 2009 | 1.028 | 124.4 ± 2.5 | |
| 2010 | 1.023 | 124.9 ± 2.5 | |
| f280 | 2008 | 0.887 | 99.1 ± 2.0 |
| 2010 | 0.892 | 100.0 ± 2.0 | |
Notes. Beams depend only on frequency and season. These include a correction to the dustsync effective frequency from the planet map and a convolution with a Gaussian which models the pointing uncertainty.
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