Table 1
Overview of the detector parameters.
| Name | Frequency | Ellipticity | FWHM | ψ pol | σw(μK) |
|
|
|||||
| 300,0 | 30 GHz | 1.7 | 32.2352′ | −22.3° | 514 |
| 300,1 | 30 GHz | 1.8 | 32.1377′ | 67.6° | 514 |
| 301,0 | 30 GHz | 1.7 | 32.2352′ | 22.3° | 514 |
| 301,1 | 30 GHz | 1.8 | 32.1377′ | −67.6° | 514 |
| 700,0 | 70 GHz | 1.7 | 13.0328′ | 22.2° | – |
| 700,1 | 70 GHz | 1.8 | 12.9916′ | −67.5° | – |
| 701,0 | 70 GHz | 1.7 | 13.0328′ | −22.2° | – |
| 701,1 | 70 GHz | 1.8 | 12.9916′ | 67.5° | – |
Notes. The first subscript denotes the horn, the second the number of the detector inside the horn. σw is the standard deviation of the Gaussian random numbers that are added to each TOD sample in simulations with white noise. Except for the ellipticities (which were exaggerated to stress-test our algorithm), the values are roughly comparable to those given in Tables 1 and 2 in Mandolesi et al. (2010). The absolute value of the individual ψpol is not relevant in the context of this paper, only their pairwise differences are.
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