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Table F.1

Summary of the spectral width of the disk-outflow/jet systems compared to the line-broadening of MUSE from Fig. 8.

Source Line Spatial resolution (mas) λcenter (Å) Line width (km s¯1) Resolved?
[O I] λ6300 2.84 71.0 6297.47 135.22 Marginally
[O I] λ6363 2.87 71.8 6360.69 135.67 Marginally
[N II] λ6548 2.86 71.5 6544.92 130.89 Marginally
DL Tau [N II] λ6583 2.56 64.0 6579.97 116.65 No
Hα 2.66 66.5 6559.97 121.22 No
[S II] λ6716 2.79 69.8 6713.38 124.87 Marginally
[S II] λ6730 2.75 68.8 6727.47 122.54 Marginally

[O I] λ6300 3.38 84.5 6297.71 160.90 Yes
[N II] λ6583 3.49 87.3 6580.21 158.72 Yes
CI Tau [S II] λ6716 3.36 84.0 6713.89 150.17 Yes
[S II] λ6730 3.43 85.8 6727.71 152.89 Yes

[O I] λ6300 3.02 75.5 6301.51 143.70 Marginally
[N II] λ6548 3.12 78.0 6550.06 143.18 Marginally
DS Tau [N II] λ6583 2.84 71.0 6585.26 129.32 Marginally
[S II] λ6716 2.59 64.8 6718.01 115.56 No
[S II] λ6730 2.94 73.5 6732.76 130.87 Marginally

IP Tau [O I] λ6300 4.30 107.5 6298.50 204.58 Yes

[O I] λ6300 5.51 137.8 6299.17 262.19 Yes
IM Lup [N II] λ6583 2.97 74.3 6581.67 135.32 Marginally

Notes. The λcenter refers to the center of the jet area where the flux is brightest.

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