On the effect of cosmic rays in bolometric cosmic microwave background measurements from the stratosphere

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Table 3:

Confidence level for bias detection with the Hausman test in cases R₁ (top three lines) and R₂ (bottom three lines), with a naively simulated noise estimation pipeline (see text).
	68%	95%	99%
s₁	100%	96%	87%
s₂	99%	93%	70%
s₃	96%	69%	39%
s₁	59%	19%	10%
s₂	48%	15%	7%
s₃	38%	8%	1.4%

Notes. The parameters s₁, s₂, and s₃ represent three different bias estimators defined in Polenta et al. (2005) (see text).

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