Table 2

Catalog of polarized sources in the ELAIS-N1 field detected with LOFAR at 146 MHz.

ID IDStokesI RApol Decpol Pp,ref Pp,st SNref SNst RMref RMst Sp,I Πref Πst
[deg] [deg] [mJy [mJy [rad m−2] [rad m−2] [mJy [%] [%]
(J2000) (J2000) beam−1] beam−1] beam−1]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
01 ILTJ162432.20 246.1327 56.8744 7.53 5.68 17 36 9.44 ± 0.03 9.46 ± 0.01 219.78 2.35 1.77
+565228.5
02 ILTJ160538.33 241.4080 54.6551 5.10 4.69 52 73 6.08 ± 0.01 6.12 ± 0.01 610.37 0.41 0.38
+543922.6
03 ILTJ155848.42 239.6998 56.4209 1.58 1.38 10 18 –5.82 ± 0.04 –5.80 ± 0.03 374.31 0.26 0.22
+562514.4
04 ILTJ161919.70 244.8342 55.6011 0.40 9 –4.70 ± 0.05 60.72 0.33
+553556.7
05 ILTJ161623.79 244.0989 55.4513 0.50 14 –20.15 ± 0.03 11.55 1.24
+552700.8
06 ILTJ161548.48 243.9340 56.3491 0.45 10 1.43 ± 0.04(*) 32.97 0.55
+562029.8
07 ILTJ161314.05 243.2815 56.1325 0.40 9 –4.86 ± 0.05 22.54 1.00
+560810.8
08 ILTJ161240.15 243.1669 53.5996 0.71 11 10.39 ± 0.04 35.96 0.95
+533558.3
09 ILTJ160909.99 242.2811 53.9092 0.80 19 7.30 ± 0.02 61.45 0.29
+535426.8
10 ILTJ160532.84 241.3855 53.2153 1.01 12 18.44 ± 0.04 30.90 1.81
+531257.4

Notes. Column 1: source name used in the present paper; Col. 2: source name used in the Stokes I map, taken from Sabater et al. (2021); Cols. 3 and 4: right ascension and declination (J2000) of the polarized source, in degrees; Cols. 5 and 6: peak polarized intensity of the source, in mJy beam−1, in the reference epoch and the stacked data, respectively; Cols. 7 and 8: S/N of the source in the reference epoch and the stacked data, respectively; Cols. 9 and 10: Faraday RM of the source and its error, in rad m−2, in the reference epoch and the stacked data, respectively (RM synthesis parameters described in Sect. 2.3); Col. 11: peak intensity of the source on the Stokes I map, taken from Sabater et al. (2021) (6′′ angular resolution), in mJy beam−1; Cols. 12 and 13: fractional polarization of the source, calculated using both the polarization and the Stokes I maps at 20′′ angular resolution, on the reference epoch and the stacked data, respectively. (*) The RM of source 06 had to be calculated separately since the peak of the Faraday spectrum is located very close to the limit of the instrumental polarization range.

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