Fig. 1.
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MUSE fields of NGC 300. The red fields are MUSE-GTO data from the Paper I pilot study. The green fields labelled P and Q are additional MUSE-GTO observations for the outer spiral arm. The cyan fields indicate ML20 fields. The magenta fields indicate the previous PN survey area of Peña et al. (2012) using the FORS2 instrument. Image: NGC 300 in Hα taken with the Wide Field Imager (ESO), programme ID 065.N-0076.
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