Table 4
Line fluxes of the DGS galaxies.
| Source name | Extract.a | Observed spectral line | Corr. factorb | ||||||
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| [C ii] 157 μm | [O i] 63 μm | [O iii] 88 μm | [O i] 145 μm | [N ii] 122 μm | [N ii] 205 μm | [N iii] 57 μm | |||
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| Compact sample | |||||||||
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| Haro 11 | 3 × 3 | 6.55 ± 0.07 (×102) | 6.44 ± 0.12 (×102) | 1.72 ± 0.03 (×103) | 50.00 ± 3.53 | 35.10 ± 2.75 | ≤ 25.44 | 2.83 ± 0.08 (×102) | − |
| Haro 2 | 5 × 5 | 8.24 ± 0.11 (×102) | 5.44 ± 0.20 (×102) | 9.72 ± 0.35 (×102) | − | − | − | − | − |
| Haro 3 | 5 × 5 | 1.03 ± 0.01 (×103) | 5.90 ± 0.27 (×102) | 1.85 ± 0.04 (×103) | 48.20 ± 4.53 | 21.40 ± 3.87 | − | 1.23 ± 0.17 (×102) | − |
| He 2-10 | 5 × 5 | 3.88 ± 0.05 (×103) | 2.52 ± 0.04 (×103) | 3.38 ± 0.05 (×103) | 1.82 ± 0.03 (×102) | − | − | 9.85 ± 1.09 (×102) | − |
| HS 0017+1055 | 3 × 3 | 4.19 ± 0.75 | − | 9.83 ± 1.38 | − | − | − | − | − |
| HS 0052+2536 | central | 43.90 ± 3.89 | 24.70 ± 4.60 | 70.70 ± 4.04 | − | − | − | − | − |
| HS 0822+3542 | central | 1.96 ± 0.55 | − | − | − | − | − | − | − |
| HS 1222+3741 | central | 2.43 ± 0.45 | − | 14.60 ± 1.54 | − | − | − | − | − |
| HS 1236+3937 | central | ≤ 3.45 | − | − | − | − | − | − | − |
| HS 1304+3529 | 3 × 3 | 26.10 ± 2.19 | − | 31.90 ± 4.86 | − | − | − | − | − |
| HS 1319+3224 | central | 2.78 ± 0.83 | − | 9.24 ± 2.06 | − | − | − | − | − |
| HS 1330+3651 | 3 × 3 | 29.20 ± 2.96 | ≤ 20.28 | 29.80 ± 2.08 | − | − | − | − | − |
| HS 1442+4250 | 3 × 3 | 12.90 ± 2.25 | − | − | − | − | − | − | − |
| HS 2352+2733 | central | ≤ 3.84 | − | 6.94 ± 1.97 | − | − | − | − | − |
| II Zw 40 | 5 × 5 | 8.49 ± 0.10 (×102) | 6.31 ± 0.26 (×102) | 3.59 ± 0.04 (×103) | 40.80 ± 4.78 | ≤ 26.52 | − | − | − |
| I Zw 18 | 3 × 3 | 10.60 ± 0.82 | 11.50 ± 2.14 | 28.40 ± 3.43 | − | − | − | − | − |
| Mrk 1089* | 5 × 5 | 8.59 ± 0.08 (×102) | 4.07 ± 0.32 (×102) | 9.38 ± 0.33 (×102) | 27.60 ± 5.00 | 35.10 ± 6.04 | − | − | 0.15 |
| Mrk 1450 | 3 × 3 | 60.50 ± 4.28 | 35.50 ± 2.77 | 2.62 ± 0.09 (×102) | − | 2.56 ± 0.65 | − | − | − |
| Mrk 153* | 3 × 3 | 53.10 ± 1.43 | 29.70 ± 7.57 | 98.90 ± 3.80 | − | − | − | − | 0.15 |
| Mrk 209* | 5 × 5 | 68.20 ± 3.55 | 38.90 ± 11.60 | 3.13 ± 0.12 (×102) | − | − | − | − | − |
| Mrk 930 | 3 × 3 | 2.18 ± 0.06 (×102) | 1.42 ± 0.12 (×102) | 4.21 ± 0.20 (×102) | 9.07 ± 0.99 | ≤ 8.31 | − | − | 0.15 |
| NGC 1140 | total | 1.19 ± 0.02 (×103) | 4.27 ± 0.20 (×102) | 1.08 ± 0.03 (×103) | 35.40 ± 3.08 | 20.90 ± 3.20 | − | − | [0.20] |
| NGC 1569* | 3 × 3 | 1.33 ± 0.01 (×104) | 7.39 ± 0.05 (×103) | 2.80 ± 0.01 (×104) | − | − | − | − | 0.15 |
| NGC 1705* | 5 × 5 /total | 3.90 ± 0.10 (×102) | 1.56 ± 0.17 (×102) | 5.46 ± 0.26 (×102) | − | − | − | − | − |
| NGC 2366* | 5 × 5 /total | 4.90 ± 0.09 (×102) | 4.60 ± 0.16 (×102) | 2.26 ± 0.01 (×103) | − | − | − | − | 0.55 |
| NGC 4214* | total | 5.42 ± 0.03 (×103) | 1.95 ± 0.05 (×103) | 4.85 ± 0.07 (×103) | 1.45 ± 0.06 (×102) | 78.90 ± 12.00 | ≤ 77.98 | − | 0.35 |
| NGC 4861* | 5 × 5 /total | 3.08 ± 0.05 (×102) | 2.23 ± 0.24 (×102) | 1.26 ± 0.02 (×103) | 16.10 ± 2.48 | − | − | − | 0.35 |
| NGC 5253 | 5 × 5 | 4.51 ± 0.01 (×103) | 2.93 ± 0.05 (×103) | 9.01 ± 0.04 (×103) | 2.06 ± 0.04 (×102) | 92.50 ± 12.10 | − | − | − |
| NGC 625* | 5 × 5 /total | 1.50 ± 0.01 (×103) | 5.69 ± 0.30 (×102) | 2.45 ± 0.03 (×103) | − | − | − | − | 0.20 |
| Pox 186 | central | 3.14 ± 0.81 | − | 33.70 ± 3.33 | − | − | − | − | − |
| SBS 0335-052 | central/ 3 × 3 | 6.61 ± 0.97 | 21.90 ± 2.25 | 43.60 ± 2.59 | − | − | − | − | − |
| SBS 1159+545 | central | 3.48 ± 0.57 | 4.86 ± 0.97 | 4.81 ± 1.22 | − | − | − | − | − |
| SBS 1211+540 | 3 × 3 | 5.48 ± 1.77 | − | − | − | − | − | − | − |
| SBS 1249+493 | 3 × 3 | 6.06 ± 1.01 | − | − | − | − | − | − | − |
| SBS 1415+437 | 3 × 3 | 36.40 ± 1.78 | 39.10 ± 3.72 | 53.20 ± 4.39 | − | − | − | − | − |
| SBS 1533+574 | 3 × 3 | 51.40 ± 2.40 | 33.20 ± 3.57 | 88.60 ± 5.06 | − | − | − | − | − |
| Tol 1214-277 | central | 4.98 ± 1.58 | 5.70 ± 1.70 | 15.10 ± 2.23 | − | − | − | − | − |
| UGC 4483 | 3 × 3/5 × 5 | 41.50 ± 5.14 | 15.60 ± 5.11 | 25.70 ± 2.67 | − | − | − | − | − |
| UM 133 | 3 × 3 | 41.40 ± 4.13 | 20.30 ± 4.10 | 24.50 ± 5.03 | − | − | − | − | − |
| UM 311* | 5 × 5 | 4.99 ± 0.08 (×102) | 2.62 ± 0.20 (×102) | 5.08 ± 0.27 (×102) | − | ≤ 11.31 | − | − | 0.60 |
| UM 448 | central | 8.00 ± 0.19 (×102) | 5.89 ± 0.27 (×102) | 1.06 ± 0.02 (×103) | 43.40 ± 2.60 | 12.20 ± 2.14 | − | − | − |
| UM 461 | 5 × 5 | 21.80 ± 2.57 | 22.70 ± 4.97 | 79.00 ± 5.91 | − | ≤ 2.04 | − | − | − |
| VII Zw 403 | 3 × 3/30 ′′ | 1.57 ± 0.05 (×102) | 42.70 ± 8.82 | 81.60 ± 8.92 | 7.36 ± 1.62 | ≤ 5.88 | − | − | − |
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| Extended sample | |||||||||
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| IC 10 | n.a. | 3.63 ± 0.02 (×10-7) | 3.40 ± 0.06 (×10-7) | 9.28 ± 0.11 (×10-7) | 1.73 ± 0.08 (×10-8) | 8.05 ± 1.05 (×10-9) | − | − | − |
| LMC-30Dor | n.a. | 2.29 ± 0.01 (×10-6) | 3.58 ± 0.02 (×10-6) | 2.12 ± 0.02 (×10-5) | 3.50 ± 0.04 (×10-7) | 5.23 ± 0.22 (×10-8) | − | − | − |
| LMC-N11A | n.a. | 3.53 ± 0.04 (×10-7) | 7.94 ± 0.06 (×10-7) | − | − | − | − | − | − |
| LMC-N11B | n.a. | 7.92 ± 0.10 (×10-7) | 1.66 ± 0.02 (×10-6) | 2.12 ± 0.04 (×10-6) | 8.33 ± 0.30 (×10-8) | 1.48 ± 0.26 (×10-8) | ≤ 1.10 (×10-8) | 1.53 ± 0.13 (×10-7) | − |
| LMC-N11C | n.a. | 4.78 ± 0.04 (×10-7) | 4.28 ± 0.04 (×10-7) | 1.89 ± 0.01 (×10-6) | − | − | − | − | − |
| LMC-N11I | n.a. | 2.12 ± 0.02 (×10-7) | 2.81 ± 0.03 (×10-7) | 1.25 ± 0.02 (×10-7) | − | − | − | − | − |
| LMC-N158 | n.a. | 9.90 ± 0.07 (×10-7) | 1.03 ± 0.01 (×10-6) | 2.75 ± 0.02 (×10-6) | − | − | − | − | − |
| LMC-N159 | n.a. | 1.30 ± 0.01 (×10-6) | 1.56 ± 0.01 (×10-6) | 5.06 ± 0.03 (×10-6) | 2.18 ± 0.03 (×10-7) | 2.92 ± 0.15 (×10-8) | ≤ 1.73 (×10-8) | − | − |
| LMC-N160 | n.a. | 1.35 ± 0.01 (×10-6) | 3.40 ± 0.02 (×10-6) | 9.79 ± 0.05 (×10-6) | 3.49 ± 0.03 (×10-7) | − | − | − | − |
| NGC 4449 | n.a. | 1.60 ± 0.01 (×10-7) | 8.74 ± 0.19 (×10-8) | 2.61 ± 0.03 (×10-7) | 6.49 ± 0.85 (×10-9) | 5.34 ± 1.20 (×10-9) | − | − | − |
| NGC 6822 | n.a. | 1.43 ± 0.01 (×10-7) | 1.36 ± 0.04 (×10-7) | 7.33 ± 0.09 (×10-7) | 7.76 ± 1.03 (×10-9) | ≤ 6.00 (×10-9) | − | − | − |
| SMC-N66 | n.a. | 1.86 ± 0.01 (×10-7) | 5.14 ± 0.04 (×10-7) | 6.61 ± 0.08 (×10-7) | − | − | − | − | − |
Notes. Fluxes are in 10-18 W m-2 for compact and fully mapped extended galaxies (compact sample), and surface brightness in W m-2 sr-1 for partially mapped extended galaxies (extended sample). Upper limits are 3σ levels. Beam sizes are 9.5′′ at 57, 63, and 88 μm, 10′′ at 122 μm, 11′′ at 145 μm, 11.5′′ at 157 μm, and 14.5′′ at 205 μm. We note that for UM 311 and NGC 4861, the PACS fluxes and correction factors are measured at the position of the main H ii complexes. The [C ii] maps cover more of the system/galaxy, with a total flux of 929 and 516 × 10-18 W m-2, respectively.
Extraction methods for the compact sample: central, 3 × 3, 5 × 5, aperture photometry (radius in ′′), or total of the line map (see Sect. 2.1.5 for details). For the extended sample, we indicate the peak surface brightness of the region mapped. The peak position is shown by a dark cross on the line maps in Appendix B).
Correction factor derived from the PACS 100 μm maps to apply in order to account for the fraction of line emission outside of the coverage of our observations. All galaxies with emission at the edges of the PACS observations are indicated with the symbol (*), and we report correction factors if missing more than 15% of the total flux. For NGC 1140, this factor has to be applied for all fluxes but [C ii] because it corrects for a different line coverage (see Sect. 2.1.7 for details).
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