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Table 1.

Coordinates and electron densities (ne) of the sources depicted in Figs. 2 and 3.

ID RA Dec ne vr. err.
(hh:mm:ss) (dd:mm:ss) (cm−3) (km s−1) (km s−1)
A1 05:38:45.58 −69:06:49.4 488 −35.4 6.9
A2 05:38:45.80 −69:06:52.9 590 −24.1 5.3
A3 05:38:45.97 −69:06:57.1 670 −41.5 2.6
A4 05:38:46.66 −69:06:52.1 107 11.5 15.7
B1 05:38:47.65 −69:06:27.3 182 −27.2 10.3
B2 05:38:48.09 −69:06:29.5 1132 −10.3 0.8
B3 05:38:48.41 −69:06:32.3 517 −12.3 2.4
B4 05:38:48.44 −69:06:34.8 392 −133.7 34.2
B5 05:38:48.96 −69:06:33.0 208 −15.5 2.4

Notes. The electron densities are calculated as averages within a 1″ aperture centered on each target, using the MUSE density map (Fig. 1). The average ne of the sky surrounding the targets, which is approximately 180 cm−3, has been subtracted from the measurements. The average radial velocities (vr.) and dispersions (err.) of the residual [S II] λλ 6716, 6731 lines, following background filtering (as described in Sect. 4), within a 1″ aperture, are listed in the last two columns.

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