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Fig. 5


Contours of the two detections in CL 0926+1242 superimposed on the HST ACS/F814W image. We applied a small shift of 0.4′′ in RA and 0.3′′ in Dec between the CO and optical images, reflecting the GSC1 catalog uncertainties in absolute astrometry used by HST at the time of the observations. The contours are at 50%, 70%, and 90% of the peak maximum (1.6 Jy km s-1).

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