Table 1.
Radio continuum and infrared properties of the detected galaxies.
| Galaxy | RA | Dec | Morphology | MS | S20 cm | FW3PAH | qW3PAH | log(FTIR) | qTIR |
 |
|---|---|---|---|---|---|---|---|---|---|---|
| (h m s) | (° ′ ″) | (mJy) | (mJy) | (W m2) | ||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | |
| NGC 2397 | 07:21:19.9 | −69:00:5.30 | SB(s)b | 2 | 50 ± 2 | 482 ± 23 | 2.8 | −9.3 | 2.4 | ... |
| NGC 2442 | 07:36:23.8 | −69:31:51.0 | SAB(s)bc pec | 2 | 327 ± 11 | 473 ± 23 | 2.0 | −9.3 | 1.6 | ... |
| ESO 059-G012 | 07:38:32.0 | −68:46:14.4 | Sa | 0 | 0.2 ± 0.1 | 17 ± 1 | 3.7 | −10.6 | 3.5 | ... |
| NGC 2434 | 07:34:51.6 | −69:17:02.9 | S0 | 0 | 2.0 ± 0.1 | ... | ... | ... | ... | ... |
| ESO 263-G033 | 10:24:47.46 | −43:57:51.60 | (R)SA0(s)? | 0.3 ± 0.1 | 0.5 ± 0.3 | 2.0 | ... | ... | ... | |
| NGC 3256 | 10:27:51.2 | −43:54:13.4 | Sb(s) pec | 3 | 476 ± 1 | 2311 ± 106 | 2.5 | −8.8 | 1.9 | −0.9 ± 0.01 |
| PGC 087403 | 10:28:25.8 | −44:16:17.0 | dIrr | 2 | 0.5 ± 0.1 | ... | ... | ... | ... | ... |
| LEDA 3097821 | 10:28:59.6 | −44:41:12.0 | ... | ... | 0.4 ± 0.1 | ... | ... | ... | ... | ... |
| NGC 3256B | 10:29:01.0 | −44:24:10.4 | SB(s)bc | 2 | 38 ± 1 | 142 ± 7 | 2.4 | −9.8 | 2.0 | −0.8 ± 0.2 |
| NGC 3261 | 10:29:01.4 | −44:39:24.6 | SB(rs)b | 2 | 65 ± 1 | 145 ± 9 | 2.2 | ... | ... | ... |
| NGC 3256C | 10:29:05.7 | −43:50:57.4 | SB(rs)d | 2 | 23 ± 1 | 111 ± 5 | 2.5 | −9.9 | 2.1 | −1.5 ± 0.4 |
| NGC 3263 | 10:29:13.3 | −44:07:22.5 | SB(rs)cd | 2.5 | 148 ± 1 | 450 ± 22 | 2.3 | −9.3 | 1.8 | −1.2 ± 0.1 |
| ESO 263-G044 | 10:29:29.5 | −44:16:06.0 | ... | 2 | 2.3 ± 0.1 | 3.0 ± 0.2 | 2.0 | −11.2 | 1.8 | ... |
| NGC 3256A | 10:25:51.0 | −43:44:53.0 | dIrr | 2 | 0.2 ± 0.1 | 1.2 ± 0.2 | 2.6 | −11.2 | 2.4 | ... |
| ESO 263-G045 | 10:29:34.5 | −44:22:38.0 | ... | ... | 1.4 ± 0.2 | ... | ... | ... | ... | ... |
| LEDA 537146 | 10:30:04.9 | −44:27:13.0 | dE? | ... | 1.0 ± 0.1 | ... | ... | ... | ... | ... |
| ESO 263-G046 | 10:30:15.4 | −44:18:28.0 | SB(s)d | 2.5 | 0.7 ± 0.1 | 3.9 ± 0.2 | 2.5 | −11.2 | 2.3 | ... |
| NGC 6215 | 16:51:06.80 | −58:59:36.0 | SA(s)c | 2.5 | 293 ± 1 | 887 ± 41 | 2.4 | −9.0 | 1.9 | −1.2 ± 0.1 |
| NGC 6221 | 16:52:46.32 | −59:13:00.0 | SB(s)c | 2.5 | 353 ± 1 | 1951 ± 91 | 2.6 | −8.7 | 2.1 | −1.4 ± 0.1 |
| ESO 138-G004 | 16:52:48.40 | −58:56:46.1 | ... | ... | 0.3 ± 0.2 | ... | ... | ... | ... | ... |
| ESO 138-G005 | 16:53:53.37 | −58:46:40.8 | ... | ... | 4.4 ± 0.2 | ... | ... | ... | ... | ... |
| ESO 138-G001 | 16:51:20.26 | −59:14:04.2 | ... | ... | 36 ± 19 | ... | ... | ... | ... | ... |
Notes. Derived sample properties. From left to right: (1) galaxy name, (2) J2000 galaxy co-ordinates, (3) morphological type from NED, (4) merger stage (MS) based on Haan et al. (2011), (5) integrated 20-cm flux density, (6) infrared flux density, (7) qW3PAH parameter, (8) TIR flux estimated using Cluver et al. (2017), (9) qTIR parameter, and (10) in-band spectral index.‘*’ indicates detected background galaxies.
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