Table 3
Statistics of the SFR distributions.
| Object |
|
|
|
|
Σobs(P5) | Σobs(P95) | Σcorr(P5) | Σcorr(P95) | A V,median |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
|
|
|||||||||
| IRAS06206-6315 | 0.1 | 0.2 | 1.2 (0.6) | 1.5 (2.3) | 0.1 | 1.5 | 0.1 | 4.5 | 6.4 |
| NGC 2369 | 1.4 | 3.9 | 5.0 (2.5) | 13.8 (21.5) | 0.3 | 7.8 | 0.6 | 60.7 | 18.5 |
| NGC 3110 | 1.0 | 1.6 | 2.2 (0.8) | 2.6 (2.6) | 0.3 | 3.0 | 0.5 | 7.6 | 8.8 |
| NGC 3256† | 2.4 | 3.4 | 6.6 (3.1) | 10.6 (8.1) | 0.5 | 9.0 | 0.5 | 18.6 | 4.9 |
| ESO320-G030 | 1.4 | 1.8 | 3.0 (1.1) | 3.6 (3.3) | 0.4 | 3.8 | 0.5 | 8.7 | 5.1 |
| IRAS12112+0305 | 0.2 | 0.3 | 1.8 (1.0) | 2.8 (3.4) | 0.1 | 2.2 | 0.1 | 6.4 | 6.4 |
| IRASF12115-4656 | 0.7 | 1.0 | 1.6 (0.6) | 2.9 (3.3) | 0.4 | 2.1 | 0.5 | 7.5 | 7.9 |
| NGC 5135 | 1.5 | 2.3 | 6.2 (2.6) | 8.6 (6.8) | 0.3 | 7.7 | 0.4 | 19.7 | 8.0 |
| IRAS14348-1447 | 0.1 | 0.2 | 1.9 (0.9) | 3.2 (3.2) | <0.1 | 1.6 | 0.1 | 4.8 | 6.3 |
| IRASF17138-1017 | 1.5 | 2.8 | 9.4 (4.3) | 12.6 (8.3) | 0.4 | 12.5 | 0.5 | 23.3 | 6.6 |
| IRAS17208-0014 | 0.2 | 0.3 | 2.9 (2.0) | 4.3 (6.4) | 0.1 | 5.1 | 0.1 | 12.6 | 5.4 |
| IC 4687 | 1.9 | 3.3 | 5.7 (2.8) | 8.7 (5.4) | 0.4 | 7.9 | 0.5 | 16.0 | 5.4 |
| IRAS21130-4446 | 0.2 | 0.3 | 2.4 (1.0) | 1.7 (2.7) | <0.1 | 3.0 | <0.1 | 6.1 | 4.2 |
| NGC 7130 | 0.6 | 0.8 | 4.9 (3.5) | 4.9 (13.4) | 0.3 | 5.3 | 0.3 | 17.4 | 5.4 |
| IC5179 | 0.7 | 0.7 | 5.2 (1.7) | 2.8 (5.3) | 0.3 | 3.0 | 0.3 | 6.1 | 4.1 |
| IRAS22491-1808 | 0.1 | 0.2 | 1.1 ( 0.6) | 1.2 (1.7) | <0.1 | 1.6 | 0.1 | 4.6 | 6.4 |
| IRAS23128-5919 | 0.2 | 0.2 | 4.0 (3.0) | 4.6 (9.8) | <0.1 | 3.5 | 0.1 | 8.1 | 6.2 |
|
|
|||||||||
| LIRGs | 1.2 | 1.7 | 2.1 (2.6) | 4.5 (8.8) | 0.3 | 6.8 | 0.4 | 17.0 | 5.3 |
| ULIRGs | 0.2 | 0.2 | 0.7 (2.0) | 1.6 (6.6) | <0.1 | 2.8 | 0.1 | 6.8 | 6.5 |
Notes. Statistics of the star formation rate surface density, ΣSFR, distributions. Columns (2) and (3): median ΣSFR values of the observed (2) and extinction-corrected (3) spaxel-by-spaxel distributions. Columns (4) and (5): weighted mean ΣSFR values of the observed (4) and extinction-corrected (5) distributions. The standard deviation of each distribution is shown in brackets. Columns (6) to (9): 5th and 95th percentiles of the distributions. Column (10): medianAV from the spaxel-by-spaxel extinction distributions (Piqueras López et al. 2013). All the quantities are expressed in [M⊙ yr-1 kpc-2], except AV, which is expressed in magnitudes.
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