VLT spectropolarimetry of the optical transient in NGC 300 - Evidence of asymmetry in the circumstellar dust

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Table 2:

Dominant axis least squares fit parameters.
Date	U₀	$\theta$	$\sigma$	r_xy	$\chi^2$ /d.o.f.
	(%)	(deg)	(%)
01-07-2008	-0.42 (0.02)	69.6 (0.4)	0.19	-0.94	432/180
08-07-2008	-0.46 (0.02)	67.6 (0.5)	0.23	-0.92	333/179
01-07-2008	-0.43 (0.02)	68.6 (0.4)	0.20	-0.94	463/180
08-07-2008	-0.45 (0.02)	68.6 (0.5)	0.22	-0.92	311/179

Notes. Values in parenthesis are the statistical rms uncertainties.
The lower part of the table reports the same values after rotation to the average dominant axis ( $\theta = 68.6$ degrees).

Source LaTeX | All tables | In the text

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