SVS13 protostellar cluster: Comparison of our CS(2–1) NOEMA-SOLIS map (colour scale and white contours) and the spatial distribution of the [OI] gas observed at 63 μm with SOFIA (black contours; some contours are not closed due to the FoV of the SOFIA observations). The contours correspond to three levels between (0.068–0.400) × 10⁻¹³ erg s⁻¹ cm⁻², as in Figure 5 by Sperling et al. (2020). The FWHM beam size of the SOFIA observations is 5″.4. The dashed lines indicate the direction of the two main jets: (i) PA ≃ 130^ˆ (connecting SVS13-A and HH11) and (ii) PA ∼ 155^ˆ (traced by H₂, and CO bullets; see text).