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Fig. A.1

image

MUSE data of multiply lensed background sources of MACS 1206. The vertical black lines indicate the positions of the emission lines based on the best estimate of the systemic redshift. The gray area shows the rescaled variance obtained from the data reduction pipeline; the flux is given in units of 10-20 erg s-1 cm-2 Å-1. The image cutouts in each panel have 2″ across and are extracted from the CLASH color image. The white circles show the HST counterparts or are centered at the position of the MUSE emission in the cases of no apparent counterparts.

This figure is made of several images, please see below:

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