Microlensing in H1413+117: disentangling line profile emission and absorption in a broad absorption line quasar

Free Access

Table 3:

Polarimetry of the four images.
	A	B	C	D	ABC
p
1999/03	1.6 $\pm$ 0.5	2.3 $\pm$ 0.5	1.8 $\pm$ 0.5	2.9 $\pm$ 0.5	1.8 $\pm$ 0.3
1999/06	-	-	-	1.0 $\pm$ 0.6	0.9 $\pm$ 0.3
2008/05	1.4 $\pm$ 0.1	2.4 $\pm$ 0.1	1.2 $\pm$ 0.1	2.0 $\pm$ 0.1	1.65 $\pm$ 0.04
$\theta$
1999/03	75 $\pm$ 9	65 $\pm$ 6	71 $\pm$ 8	102 $\pm$ 5	70 $\pm$ 4
1999/06	-	-	-	103 $\pm$ 18	87 $\pm$ 11
2008/05	72 $\pm$ 2	79 $\pm$ 1	69 $\pm$ 3	96 $\pm$ 2	75 $\pm$ 1

Notes. The polarization degree p is given in percent and the polarization position angle $\theta$ in degree, East of North. The data obtained in 1999 are from Chae et al. (2001).

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.