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Table 1.

Compendium of the sub-millimetre Crab nebula polarisation angle measurements in Galactic coordinates for WMAP (Weiland et al. 2011), XPOL (Aumont et al. 2010), Planck-LFI (Planck Collaboration XXVI 2016), and Planck-HFI and NIKA (Ritacco et al. 2018).

Experiment ν (GHz) Beam ψGal (deg) Statistical Systematic (deg)

size (deg) Ground EB TB
WMAP 23 53′ −88.5 0.1 1.5
33 40′ −87.7 0.1 1.5
41 31′ −87.3 0.2 1.5
61 21′ −87.7 0.4 1.5
94 13′ −88.7 0.7 1.5
XPOL 90 27″ −88.8 ( ⋆ ) 0.2 0.5
Planck-LFI 30 33′ −89.26 0.25 0.5
44 27′ −88.65 0.79 0.5
70 13′ −87.49 1.33 0.5
Planck-HFI 100 10′ −87.52 0.16 1.00 0.49 0.21
143 7′ −86.61 0.21 1.00 0.32 0.19
217 5′ −87.93 0.25 1.00 0.36 0.62
353 5′ −86.76 0.52 1.00
NIKA 150 18″ −84.3 ( • ) 0.7 2.3

Notes. In the case of Planck-HFI, the so-called ground systematic uncertainties come from Rosset et al. (2010). The systematic uncertainties called EB and TB are derived from the and minimisation presented in Planck Collaboration Int. XLVI (2016).

( ⋆ )Convolved with a 10′ Gaussian.

( • )Computed with aperture photometry techniques within 9′.

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