WSRT Faraday tomography of the Galactic ISM at λ ~ 0.86 m - I. The GEMINI data set at (l, b) = (181°, 20°)

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Volume 494 / No 2 (February I 2009)

A&A, 494 2 (2009) 611-622

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Table 2:

Properties of the polarized point sources we found in our data. Shown are the equatorial coordinates (J2000.0) of the source in decimal degrees, the RM that we fitted and its error (both in rad/m²), the reduced $\chi ^2$ ( $\chi ^2_{{\rm red}}$ ) of the fit, the maximum $P(\mathcal{R})$ along the line of sight and the total intensity I (both in mJy), and the polarization fraction (in %).
(RA, Dec)	RM	$\chi ^2_{{\rm red}}$	$P({\mathcal{R}})_{{\rm max}}$	I	$P({\mathcal{R}})_{{\rm max}}$ /I
( $^\circ$ , $^\circ$ )	[rad/m²]		[mJy]	[mJy]	%
(113.60, 35.12)	-27.6 $\pm$ 0.1	0.5	23.4	329	7.1
(113.25, 36.92)	14.2 $\pm$ 0.3	0.6	6.1	177	3.4
(113.34, 39.09)	9.6 $\pm$ 0.4	0.7	7.9	236	3.3
(113.20, 38.69)	11.7 $\pm$ 0.4	0.8	5.8	184	3.2
(112.84, 36.38)	14.3 $\pm$ 0.5	1.1	6.9	337	2.0
(112.04, 35.11)	8.7 $\pm$ 0.4	0.8	4.6	214	2.2
(111.91, 40.23)	18.9 $\pm$ 0.4	1.1	6.2	151	4.1
(111.54, 40.17)	13.8 $\pm$ 0.5	1.4	5.7	272	2.1
(111.32, 35.69)	6.5 $\pm$ 0.3	0.5	10.9	277	3.9
(111.42, 40.07)	11.8 $\pm$ 0.3	0.9	5.3	152	3.5
(111.24, 39.36)	16.3 $\pm$ 0.6	1.4	7.0	333	2.1
(111.02, 38.05)	13.3 $\pm$ 0.2	0.5	10.0	375	2.7
(110.77, 32.65)	-9.8 $\pm$ 0.7	2.8	5.4	232	2.3
(110.68, 32.51)	-7.8 $\pm$ 0.6	2.1	4.8	242	2.0
(110.74, 39.97)	9.4 $\pm$ 0.3	0.6	11.8	239	4.9
(110.29, 35.82)	5.7 $\pm$ 0.5	0.9	6.3	258	2.4
(108.90, 38.64)	19.0 $\pm$ 0.4	1.9	4.5	197	2.3
(108.42, 34.52)	20.5 $\pm$ 0.2	1.0	17.4	828	2.1
(108.31, 36.93)	22.2 $\pm$ 0.2	1.0	5.3	214	2.5
(108.27, 36.95)	25.7 $\pm$ 0.6	2.7	4.4	210	2.1
(106.30, 37.31)	-12.7 $\pm$ 0.4	1.2	4.4	195	2.3
(105.76, 38.38)	-12.3 $\pm$ 0.6	1.4	3.1	150	2.0
(104.81, 35.88)	-33.4 $\pm$ 0.4	1.6	15.1	625	2.4

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