Table 1.
Line flux and EQW of 3.3 μm PAH and Brα and the Fν(4.3 μm)/Fν(2.8 μm) color measured in the 4.4″ radius aperture.
| Object name | RA | Dec | F3.3 μm PAH | EQW3.3 μm PAH | FBrα | EQWBrα | Fν(4.3 μm)/Fν(2.8 μm) | EQW6.2 μm PAH |
|---|---|---|---|---|---|---|---|---|
| NGC0023 | 2.472551 | 25.923980 | 7.49 ± 0.55 | 0.055 ± 0.004 | 0.60 ± 0.09 | 0.008 ± 0.001 | 0.71 ± 0.02 | 0.579 ± 0.007 |
| NGC0034 | 2.776792 | −12.107964 | 4.32 ± 0.23 | 0.046 ± 0.002 | 0.29 ± 0.09 | 0.005 ± 0.002 | 0.93 ± 0.02 | 0.453 ± 0.025 |
| Arp256 | 4.711997 | −10.376844 | 4.52 ± 0.10 | 0.156 ± 0.003 | 0.58 ± 0.07 | 0.030 ± 0.004 | 1.05 ± 0.07 | 0.719 ± 0.010 |
| NGC0232 | 10.690820 | −23.561306 | 3.93 ± 0.22 | 0.048 ± 0.003 | 0.33 ± 0.11 | 0.007 ± 0.002 | 0.85 ± 0.02 | 0.549 ± 0.007 |
| MCG+12-02-001 | 13.516243 | 73.084991 | 10.78 ± 0.25 | 0.134 ± 0.003 | 1.68 ± 0.11 | 0.030 ± 0.002 | 1.29 ± 0.02 | 0.654 ± 0.008 |
| MCG-03-04-014 | 17.537453 | −16.852654 | 5.71 ± 0.12 | 0.115 ± 0.002 | 0.37 ± 0.12 | 0.012 ± 0.004 | 0.98 ± 0.02 | 0.665 ± 0.009 |
| ESO244-G012 | 19.534571 | −44.462093 | 6.28 ± 0.17 | 0.124 ± 0.003 | 0.79 ± 0.07 | 0.023 ± 0.002 | 1.03 ± 0.02 | 0.665 ± 0.010 |
| CGCG436-030 | 20.010996 | 14.361864 | 2.60 ± 0.08 | 0.069 ± 0.002 | 0.53 ± 0.04 | 0.017 ± 0.001 | 1.81 ± 0.05 | 0.347 ± 0.008 |
| ESO353-G020 | 23.713484 | −36.137360 | 3.12 ± 0.22 | 0.048 ± 0.003 | 0.51 ± 0.00 | 0.013 ± 0.000 | 0.85 ± 0.02 | 0.544 ± 0.008 |
| RR032 | 24.097355 | −37.321678 | 4.12 ± 0.27 | 0.098 ± 0.006 | <0.09 | <0.003 | 1.02 ± 0.04 | 0.522 ± 0.010 |
| IRASF01364-1042 | 24.720614 | −10.453101 | 0.58 ± 0.08 | 0.044 ± 0.006 | <0.10 | <0.013 | 0.66 ± 0.10 | 0.392 ± 0.011 |
| IIIZw035a | 26.126998 | 17.101369 | 1.18 ± 0.06 | 0.062 ± 0.003 | <0.13 | <0.010 | 0.98 ± 0.05 | … |
Notes. The full table is available at the CDS. The line fluxes and EQWs are in units of 10−16 W m−1 and μm, respectively. The 6.2 μm PAH EQWs (μm) are from Stierwalt et al. (2013).
Mismatched pointings between the AKARI and Spitzer observations or too extended morphologies to combine the AKARI and Spitzer spectra. Other quantities for the GOALS galaxies, such as the AGN fraction (see Sect. 4.1), stellar mass, UV and IR fluxes and LIR can be found in Díaz-Santos et al. (2017), Howell et al. (2010) and Armus et al. (2009).
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