“…This happened because already first science case that motivated the construction of MUSE framed it as a discovery machine for the faintest line emitting objects. (Bacon et al, 2002); a dream that has now become reality (e.g., Bacon et al, 2021;Maseda et al, 2018;Sánchez Almeida et al, 2022). As of this writing the following software implementations for detecting and cataloguing emission lines in wide-field IFS data cuboids are freely 1 available: "Source Emission Line FInder" (SELFI; Meillier et al, 2016), ORIGIN (Mary et al, 2020), MUSELET (a wrapper of the popular imaging source detection software SExtractor and part of the MUSE Python Data Analysis Framework; Piqueras 1 Another software is CubeEx, but this programme is only available from the author on request (see the the "code availability" remark in Ginolfi et al, 2022).…”