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Table 3

Near-infrared data.

maxBCG RADec Ellipticity Ks Note
(J2000) (mag)
(1) (2) (3) (4) (5)

2596 N 01:02:00.677 – 10:33:02.46 0.056 17.57  ±  0.034 N
2596 E 01:02:02.089 – 10:32:57.99 0.045 17.22  ±  0.037 SDSS
2596 W 01:01:59.311 – 10:33:10.95 0.381 16.91  ±  0.023 SDSS
3131 N 00:34:48.040 – 00:21:32.47 0.432 19.21  ±  0.117 N/S82
3131 D1 00:34:48.421 – 00:21:35.99 0.128 17.78  ±  0.040 S82
3131 D2 00:34:47.719 – 00:21:27.19 0.208 17.51  ±  0.034 SDSS/S82
3131 L 00:34:48.333 – 00:21:29.70 0.540 19.59  ±  0.143 S82
3131 E1a 00:34:48.774 – 00:21:20.20 0.843 19.62  ±  0.164 S82
3131 E2a 00:34:48.954 – 00:21:25.16 0.219 18.97  ±  0.097 SDSS/S82
3131 E3 00:34:48.990 – 00:21:31.22 0.097 17.61  ±  0.036 SDSS/S82
3131 S1 00:34:47.521 – 00:21:45.26 0.426 17.66  ±  0.037 SDSS/S82
3131 S2 00:34:47.211 – 00:21:45.72 0.125 18.23  ±  0.055 S82
6167 N 00:24:52.655 – 00:52:01.49 0.073 19.88  ±  0.149 N/S82
8495 Nab 00:43:59.447 + 00:12:30.01 0.237 18.20  ±  0.072 ...
8495 Nbb 00:43:59.526 + 00:12:30.84 0.256 18.56  ±  0.096 ...
8495 Nc 00:43:59.488 + 00:12:30.60 0.880 17.47  ±  0.048 N/S82
8495 D 00:43:59.498 + 00:12:26.22 0.423 18.84  ±  0.121 ...
10942 N 02:17:57.382 – 09:18:18.10 0.053 18.03  ±  0.048 N
10942 W 02:17:57.166 – 09:18:05.27 0.147 19.05  ±  0.096 ...
11079 N 02:01:28.258 – 08:19:56.63 0.303 19.16  ±  0.112 N
11079 S1 02:01:28.433 – 08:20:01.79 0.398 19.10  ±  0.108 ...
11079 S2 02:01:28.493 – 08:20:11.35 0.275 19.38  ±  0.135 ...
11079 S3 02:01:28.691 – 08:20:08.10 0.444 19.24  ±  0.120 ...
11079 L 02:01:28.865 – 08:19:46.39 0.051 18.92  ±  0.093 ...
11390 N 00:03:28.911 – 11:12:53.63 0.101 19.24  ±  0.109 N
11390 E 00:03:29.109 – 11:12:52.75 0.365 19.44  ±  0.128 ...
11780 N 00:05:57.061 – 09:08:58.43 0.059 18.06  ±  0.040 N
11780 L 00:05:57.324 – 09:08:52.20 0.051 19.29  ±  0.099 ...

Notes. Column 1: the NIR source component corresponding to the SDSS maxBCG cluster field: identification number is the sequential number (Koester et al. 2007). Column 2: near-infrared position (J2000) from the GAIA aperture photometry sextractor fit (except for maxBCG 8495 component N). Column 3: ellipticity of the fitted ellipse (except for maxBCG 8495 component N). Column 4: GAIA sextractor aperture photometry Ks-band magnitude and error (except for maxBCG 8495 component N). Magnitudes are in the Vega system. Column 5: note on the component: N – component coincident with the center of the radio structure; SDSS – SDSS detection; S82 – Stripe 82 detection.

(a)

Stripe 82 images show that components E1 and E2 are two resolved components of the same edge-on galaxy.

(b)

The maxBCG 8495 Na and Nb components refer to the “double nuclear” emission region detected in the Ks-band.

(c)

The maxBCG 8495 N component refers to GAIA manual aperture photometry of a region (~2 arcsec) containing the “double nuclear” components Na and Nb.

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