Table 1.
Distribution of posterior mean noise parameters for each radiometer.
Det | α | fknee [mHz] | σ0 [mK] | ![]() |
|
---|---|---|---|---|---|
27M |
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|
30 GHz | 27S |
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28M |
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|
28S |
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|
24M |
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|
24S |
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|
44 GHz | 25M |
![]() |
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![]() |
25S |
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|
26M |
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![]() |
![]() |
![]() |
|
26S |
![]() |
![]() |
![]() |
![]() |
|
18M |
![]() |
![]() |
![]() |
– | |
18S |
![]() |
![]() |
![]() |
– | |
19M |
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![]() |
– | |
19S |
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![]() |
– | |
20M |
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![]() |
![]() |
– | |
70 GHz | 20S |
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![]() |
– |
21M |
![]() |
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![]() |
– | |
21S |
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![]() |
![]() |
– | |
22M |
![]() |
![]() |
![]() |
– | |
22S |
![]() |
![]() |
![]() |
– | |
23M |
![]() |
![]() |
![]() |
– | |
23S |
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![]() |
![]() |
– |
Notes. Error bars represent variation over time of the posterior mean values (and not the width of the posterior distribution) for any given PID.
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