Table 3.
Information on [CII] spectra acquisition and Gaussian fit.
| Individual galaxies | ||||||||
|---|---|---|---|---|---|---|---|---|
| Source | OBSID | Extraction | FWHMnarrow | FWHMbroad | log(L[CII],narrow) | log(L[CII],broad) |  |
 |
| [km s−1] | [km s−1] | [L⊙] | [L⊙] | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| Haro2 | 1342230081 | 5 × 5 | 255 ± 2 | 965 ± 193 |
 |
 |
1.21 | 0.68 |
| Haro3 (*) | 1342221892 | 5 × 5 | 223 ± 1 | 306 ± 61 |
 |
 |
1.49 | 1.10 |
| Haro11 | 1342199236 | 3 × 3 | 172 ± 7 | 570 ± 56 |
 |
 |
3.59 | 1.19 |
| He2-10 | 1342221975 | 5 × 5 | 244 ± 2 | 580 ± 33 |
 |
 |
9.60 | 0.99 |
| HS0052+2536 | 1342213134 | Central | 211 ± 23 | – |
 |
– | 0.87 | – |
| HS1222+3741 | 1342232306 | Central | 147 ± 32 | 159 ± 83 |
 |
 |
1.04 | 0.97 |
| HS1304+3529 | 1342199736 | 3 × 3 | 191 ± 17 | – |
 |
– | 0.92 | – |
| HS1330+3651 | 1342199734 | 3 × 3 | 239 ± 28 | – |
 |
– | 1.17 | – |
| HS1442+4250 | 1342208927 | 3 × 3 | 281 ± 59 | – |
 |
– | 0.79 | – |
| HS2352+2733 | 1342213133 | Central | 270 ± 50 | – |
 |
– | 0.84 | – |
| IZw18 | 1342220973 | 3 × 3 | 200 ± 23 | – |
 |
– | 0.97 | – |
| IIZw40 | 1342228253 | 5 × 5 | 236 ± 1 | – |
 |
– | 0.87 | |
| Mrk153 | 1342209015 | 3 × 3 | 257 ± 5 | – |
 |
– | 0.89 | – |
| Mrk209 | 1342199423 | 3 × 3 | 214 ± 6 | – |
 |
– | 0.92 | – |
| Mrk930 | 1342212520 | 3 × 3 | 253 ± 9 | 466 ± 201 |
 |
 |
0.90 | 0.87 |
| Mrk1089 (*) | 1342217859 | 5 × 5 | 238 ± 1 | 515 ± 58 |
 |
 |
2.71 | 1.05 |
| Mrk1450 | 1342222070 | 3 × 3 | 245 ± 14 | – |
 |
– | 0.88 | – |
| SBS0335-052 | 1342214221 | Central | 160 ± 26 | – |
 |
– | 1.04 | – |
| SBS1159+545 | 1342199228 | Central | 231 ± 30 | – |
 |
– | 0.82 | – |
| SBS1211+540 | 1342199422 | Central | 249 ± 69 | – |
 |
– | 0.78 | – |
| SBS1249+493 | 1342232266 | 3 × 3 | 244 ± 29 | – |
 |
– | 0.94 | – |
| SBS1415+437 | 1342199733 | 3 × 3 | 247 ± 11 | – |
 |
– | 0.87 | – |
| SBS1533+574 | 1342199230 | 3 × 3 | 207 ± 6 | – |
 |
– | 0.90 | – |
| UGC4483 | 1342203684 | 3 × 3 | 189 ± 12 | 279 ± 117 |
 |
 |
1.05 | 1.04 |
| UM133 | 1342212533 | 3 × 3 | 177 ± 33 | – |
 |
– | 0.78 | – |
| UM311 | 1342213288 | 5 × 5 | 241 ± 4 | 369 ± 58 |
 |
 |
1.08 | 0.86 |
| UM448 (*) | 1342222201 | 3 × 3 | 237 ± 5 | 907 ± 116 |
 |
 |
7.51 | 0.92 |
| UM461 | 1342222205 | Central | 144 ± 11 | 672 ± 355 |
 |
 |
0.93 | 0.83 |
| VIIZw403 | 1342199289 | 5 × 5 | 234 ± 6 | – |
 |
– | 1.07 | – |
| Stacking | ||||||||
| Whole sample | – | – | 247 ± 5 | 437 ± 51 |
 |
 |
1.91 | 0.81 |
| Non-det. | – | – | 240 ± 6 | 478 ± 87 |
 |
 |
1.12 | 0.76 |
Notes. Column key: (1) source name; (2) PACS Observation Identification number; (3) extraction region of the [CII] spectrum, i.e., from central spaxel, 3 × 3 or 5 × 5 spaxel coverage; (4) FWHM of the narrow component; (5) FWHM of the broad component; (6) [CII] luminosity of the narrow component; (7) [CII] luminosity of the broad component; (8) χ2 from single Gaussian fit; (9) χ2 from double Gaussian fit. Sources without FWHMbroad, L[CII],broad, and 
do not show any broad component in their spectra. For such cases, FWHMnarrow and L[CII],narrow correspond to the value obtained with a single Gaussian component. The [CII] spectrum of targets with (*) was modeled with a three-component Gaussian (see Sect. 4.1). For these sources, FWHMnarrow and L[CII],narrow are those obtained from a single Gaussian given by the sum of the two narrow components of the fit. In the bottom part of the table, first column refers to the sample used for stacking.
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