a) ArTéMiS 350 μm dust continuum mosaic of the central part of the NGC 6334 star-forming complex. The effective half-power beam width (HPBW) resolution is 8″ (or 0.07 pc at d = 1.7 kpc), a factor of >3 higher than the Herschel/HOBYS SPIRE 350 μm map (Russeil et al. 2013; Tigé et al. 2016). b) High dynamic range 350 μm dust continuum map of the same field obtained by combining the ArTéMiS high-resolution data shown in the left panel with the Herschel/SPIRE 350 μm data providing better sensitivity to large-scale emission. The effective angular resolution is also 8″ (HPBW). The crest of the main filament as traced by the DisPerSE algorithm (Sousbie 2011) is marked by the magenta curve. The footprint of the 4 × 2 subarrays of the ArTéMiS camera indicating the instantaneous field of view on the sky is shown in both panels. (The instantaneous field of view for the data taken in 2013 corresponds to the central 2 × 2 sub-arrays.)