Euclid preparation - LXXIX. Using mock low surface brightness dwarf galaxies to probe Euclid Wide Survey detection capabilities

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Fig. A.1.

Chosen MER VIS mosaic. The tile with ID 102018187 is centred on $RA = 2 ° 35' 43 \overset{″}{.} 41$ $Mathematical equation: $ \mathrm{RA} = {2\circ 35\prime 43{{\overset{\prime\prime}{.}}}41} $$ , Dec = −51° 30 00 $\overset{″}{.}$ $Mathematical equation: $ {{\overset{\prime\prime}{.}}}$$ 00. Its x- and y-axes correspond to RA and Dec, respectively. Its side length is 32′ (for a description of the tiling scheme see Euclid Collaboration: Romelli et al. 2026). Data from this tile will be publicly available as part of the Euclid first data release (DR1).

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