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Table A.1.

Extended sources in the Abell 209 MGCLS field.

(1) (2) (3) (4) (5) (6) (7) (8)
R.A. Dec. Sint ΔSint Ipeak LAS Optical ID z
(deg) (deg) (mJy) (mJy) (mJy beam−1) (″)
22.9860 −13.5807 6.049 0.053 2.411 70 - -
23.0179 −13.6651 3.549 0.031 0.530 76 7190 0.2
22.8985 −13.4712 13.067 0.063 7.516 136 4968 0.27
23.1898 −13.3511 38.210 0.044 11.053 73 - -
23.1666 −13.1819 3.503 0.040 1.367 56 6205 0.17
23.2199 −13.1328 2.074 0.066 0.807 54 8068 0.08
23.3709 −13.5798 1.993 0.029 0.716 54 1596 0.46
23.5330 −13.5719 2.742 0.030 1.061 82 WISEA J013407.92−133418.8 -
22.9890 −13.7451 3.618 0.056 1.742 107 4559 0.2
22.5779 −13.8580 0.855 0.016 0.563 37 591 0.36
22.5694 −13.8677 1.383 0.024 0.271 43 - -
22.7784 −13.0524 26.687 0.125 4.139 94 WISEA J013106.83−130308.7 -
22.7566 −13.3371 1.705 0.023 0.441 54 1353 0.34
22.6263 −13.4913 26.158 0.029 16.544 76 4158 0.3
23.4957 −13.2933 3.019 0.027 0.767 89 WISEA J013358.96−131736.1 0.1
22.5028 −13.5075 1.689 0.033 0.430 115 - -
23.3231 −13.6783 1.387 0.032 0.356 72 - -
23.0368 −13.3279 8.527 0.026 4.004 68 WISEA J013208.83−131940.4 -
22.9934 −14.1088 4.678 0.027 0.286 74 WISEA J013158.40−140631.7 -
22.9494 −13.9215 6.061 0.019 2.928 33 WISEA J013147.85−135517.5 -
23.3539 −13.3721 1.959 0.019 0.838 94 - -
22.6013 −13.1741 1.300 0.021 0.889 44 WISEA J013024.30−131026.7 -
23.3064 −13.0585 79.000 0.083 18.792 468 WISE J013313.50−130330.5 -
22.5031 −13.4747 13.570 0.016 7.594 58 WISEA J013000.74−132828.9 -
23.5757 −13.9423 6.193 0.028 1.196 93 WISEA J013418.18−135632.2 -
23.5998 −13.5860 1.831 0.012 0.827 41 WISEA J013423.94−133509.6 -
22.4480 −13.2866 28.055 0.026 8.629 65 - -
23.5316 −13.8162 25.822 0.019 10.615 47 WISEA J013407.58−134858.4 -
22.9680 −13.6162 20.589 0.049 12.144 83 164 0.18
23.4633 −13.6041 2.668 0.018 0.857 40 - -
22.6359 −13.8971 4.942 0.013 3.103 35 WISEA J013032.61−135349.6 -
22.6052 −14.0115 1.900 0.029 0.327 182 WISEA J013025.31−140042.5 -
22.9408 −13.6772 0.497 0.013 0.127 46 6812 0.19

Notes. Cols: (1–2) Source J2000 R.A. and Dec. – the position is that of the optical host, or the flux-weighted centroid if no optical host is identified; (3–4) MeerKAT 1.28 GHz integrated flux density and its uncertainty; (5) MeerKAT 1.28 GHz peak brightness; (6) Largest angular size; (7) optical host identifier where known – number-only IDs are from DECaLS; (8) Optical host redshift.

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