Fig. 2.
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Lyα maps of the close environments of GS10578 (left) and GS551 (right). They trace the emitting gas with v ∈ [ − 200, 200] km s−1 observed with MUSE. The cyan (orange) contours indicate the Lyα emission at 4σ in velocity bins of 400 km s−1, from −1400 to +1400 km s−1. The cross symbols identify the (NIRSpec) AGN positions. The coordinate grids highlight the different rotation of MUSE data with respect to the standard north-east up-left configuration.
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