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Fig. 4.
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J2347-1856 EVN 4.9 GHz data. The source is not yet rejected as a milli-lens but has strong indications to be a CSO. The contours start at four times the image rms noise of 0.296 mJy/beam and increase by factors of two. The restoring beam size is 1.55 × 4.44 mas at 68.91° PA. The source is not detected at 22.2 GHz.
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