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Table C.2

High-resolution MIR line fluxes in the compact galaxies of the DGS.

Source name Main observed spectral lines HR/LR

[S iv] 10.5 μm [Ne ii] 12.8 μm [Ne iii] 15.6 μm [S iii] 18.7 μm [S iii] 33.5 μm

Haro 3 4.08 ± 0.17 (×102) 3.52 ± 0.13 (×102) 9.84 ± 0.74 (×102) 5.03 ± 0.39 (×102) 8.51 ± 0.24 (×102) 1.08
Haro 11* 4.94 ± 0.11 (×102) 3.27 ± 0.09 (×102) 1.12 ± 0.05 (×103) 5.31 ± 0.29 (×102) 8.17 ± 0.70 (×102) 1.04
He 2-10 3.27 ± 0.13 (×102) 3.80 ± 0.13 (×103) 1.56 ± 0.05 (×103) 2.67 ± 0.19 (×103) 3.17 ± 0.10 (×103) 0.88
HS 0822+3542* 6.43 ± 0.45 0.24 2.63 ± 0.21 1.32 ± 0.22 0.92
HS 1442+4250* 8.21 ± 0.30 0.51 3.83 ± 0.68 1.69 ± 0.59 3.10 ± 1.03 1.19
II Zw 40 2.00 ± 0.10 (×103) 73.52 ± 7.93 1.41 ± 0.09 (×103) 5.21 ± 0.22 (×102) 7.82 ± 0.21 (×102) 0.97
I Zw 18 5.69 ± 1.42 2.91 7.89 ± 1.02 5.04 ± 1.29 3.94 ± 0.91 1.17
Mrk 153 24.01 ± 5.47 3.91 ± 0.77 31.22 ± 1.72 14.19 ± 2.32 28.89 ± 6.97 0.99
Mrk 209* 85.71 ± 2.88 2.45 ± 0.31 54.49 ± 1.74 24.34 ± 1.49 49.69 ± 5.70 1.07
Mrk 930 1.39 ± 0.05 (×102) 39.39 ± 2.44 2.12 ± 0.06 (×102) 94.43 ± 4.98 1.28 ± 0.11 (×102) 1.12
Mrk 1450* 72.84 ± 1.22 9.18 ± 0.72 93.06 ± 3.32 43.88 ± 1.54 70.17 ± 17.05 0.98
NGC 1140 1.80 ± 0.10 (×102) 1.83 ± 0.09 (×102) 6.28 ± 0.40 (×102) 3.31 ± 0.17 (×102) 4.34 ± 0.14 (×102) 1.16
NGC 1569 2.47 ± 0.03 (×103) 3.05 ± 0.27 (×102) 3.24 ± 0.13 (×103) 1.31 ± 0.05 (×103) 1.85 ± 0.06 (×103) 0.96
SBS 0335-052* 14.75 ± 0.37 0.72 ± 0.09 12.37 ± 0.74 3.49 ± 1.05 4.70 ± 1.58 0.71
SBS 1159+545* 5.10 2.19 2.97 4.23 12.83 n.a.
SBS 1415+437* 12.02 ± 0.92 2.31 ± 0.29 11.33 ± 0.99 7.58 ± 1.20 14.04 ± 3.42 0.81
Tol 1214-277 8.86 ± 0.47 1.56 5.57 ± 0.55 2.99 11.06 0.89
UM 448 2.32 ± 0.04 (×102) 3.14 ± 0.12 (×102) 6.38 ± 0.25 (×102) 3.21 ± 0.12 (×102) 4.92 ± 0.21 (×102) 0.92
UM 461* 46.71 ± 0.90 1.58 ± 0.39 29.11 ± 1.24 8.71 ± 0.80 12.64 ± 4.60 0.86
NGC 625 5.72 ± 0.07 (×102) 1.66 ± 0.05 (×102) 7.46 ± 0.26 (×102) 4.40 ± 0.15 (×102) 7.78 ± 0.39 (×102) n.a.
UM 311 36.80 ± 2.91 43.77 ± 13.69 1.03 ± 0.05 (×102) 76.28 ± 5.09 59.99 ± 14.60 n.a.
VII Zw 403 14.47 ± 1.42 5.09 ± 0.34 23.05 ± 2.60 18.49 ± 2.88 13.60 n.a.
Source name Other observed spectral lines

[Ar ii] 6.99 μm [Ne v] 14.3 μm [O iv] 25.9 μm [Si ii] 34.8 μm [Ne iii] 36.0 μm

Haro 3 14.50 17.93 ± 5.00 3.99 ± 0.24 (×102) 1.17 ± 0.29 (×102)
Haro 11* 5.29 43.90 ± 7.84 5.58 ± 0.45 (×102) 1.92 (×102)
He 2-10 20.84 79.15 ± 25.14 1.93 ± 0.04 (×103) 2.92 (×102)
HS 0822+3542* 1.02
HS 1442+4250* 0.43 2.37 ± 0.74 3.40 ± 1.39 7.32
II Zw 40 7.46 79.36 ± 11.53 3.68 ± 0.35 (×102) 1.74 ± 0.39 (×102)
I Zw 18 4.02 4.08 4.37 10.87
Mrk 153 3.45 5.10 ± 1.92 23.78 ± 6.17 15.73
Mrk 209* 1.87 13.13 ± 2.81 32.37 ± 4.07 16.53 ± 7.43
Mrk 930 3.29 12.02 ± 2.65 1.27 ± 0.12 (×102) 34.56 ± 13.98
Mrk 1450* 1.04 8.31 ± 0.88 30.72 ± 5.42 15.28
NGC 1140 9.94 19.84 ± 3.91 2.71 ± 0.15 (×102) 33.81 ± 16.15
NGC 1569 8.18 3.19 ± 0.15 (×102) 1.15 ± 0.03 (×103) 5.77 (×102)
SBS 0335-052* 1.63 5.22 ± 1.15 10.55 17.39
SBS 1159+545* 3.64 2.35 13.85 18.92
SBS 1415+437* 1.17 6.51 ± 2.02 17.77 ± 3.91 7.60
Tol 1214-277* 0.75 5.43 ± 2.08 8.89
UM 448 5.64 30.85 ± 6.35 4.92 ± 0.21 (×102) 77.59
UM 461* 0.72 2.77 ± 0.90 8.76 ± 2.71 20.95
NGC 625 31.40 3.89 1.85 ± 0.12 (×102) 68.04 ± 22.33
UM 311 2.55 6.39 ± 2.62 56.23 ± 5.82 17.00
VII Zw 403 5.13 1.78 12.35 16.00

Notes. Fluxes are in 10-18 W m-2. Upper limits are given at 2σ. The symbol

(*)

indicates point-like sources reduced with the optimal extraction method. The other sources are extracted from the full apertures. We note that the observation of Pox 186 (AOR key 9007360) is not included because it is not centered on the source.

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