Table 1.
Distances, 1.4 GHz fluxes, 150 MHz fluxes, and luminosities for all γ-ray emitting SFGs known.
| Galaxy | DL | F1.4 GHz | F150 MHz | log(Lγ) | log(L1.4 GHz) | log(L150 MHz) |
|---|---|---|---|---|---|---|
| [Mpc] | [mJy] | [mJy] | [erg s−1] | [W Hz−1] | [W Hz−1] | |
| M 31 | 0.77 ± 0.04 (a) | 8600 ± 1100 (b) | 219 000 ± 21 000 (g) | 38.10 ± 0.12 | 21.28 ± 0.14 | 22.19 ± 0.06 |
| NGC 253 | 3.56 ± 0.26 (a) | 5677 ± 81 | 16 600 ± 1400 (h) | 40.01 ± 0.07 | 21.93 ± 0.06 | 22.40 ± 0.07 |
| SMC | 0.060 ± 0.003 (a) | 57 000 ± 5000 (c) | 258 300 ± 67 300 (i) | 37.04 ± 0.05 | 19.39 ± 0.06 | 20.05 ± 0.12 |
| M 33 | 0.91 ± 0.04 (a) | 3300 ± 500 (b) | 5600 ± 1800 (m) | 38.30 ± 0.09 | 20.51 ± 0.08 | 20.74 ± 0.14 |
| NGC 1068 | 10.1 ± 1.8 (a) | 5027 ± 7 | 21230 ± 3400 (n) | 40.90 ± 0.16 | 21230 ± 3400 | 23.41 ± 0.17 |
| LMC | 0.050 ± 0.003 (a) | 426 000 ± 29 000 (d) | 1 450 100 ± 246 600 (i) | 37.77 ± 0.05 | 20.10 ± 0.06 | 20.64 ± 0.09 |
| NGC 2146 | 17.2 ± 3.2 (a) | 1082 ± 3 | 4040 ± 90 (o) | 40.76 ± 0.18 | 22.58 ± 0.16 | 23.15 ± 0.16 |
| NGC 2403 | 3.18 ± 0.18 (a) | 148 ± 0.5 | 970 ± 50 (j) | 39.17 ± 0.11 | 20.25 ± 0.05 | 21.07 ± 0.05 |
| M 82 | 3.53 ± 0.26 (a) | 7389 ± 13 | 15 840 ± 790 (j) | 40.20 ± 0.07 | 22.04 ± 0.06 | 22.37 ± 0.07 |
| NGC 3424 | 25.6 ± 1.8 (a) | 71 ± 1.8 | 230 ± 30 (j) | 40.92 ± 0.13 | 21.75 ± 0.06 | 22.26 ± 0.08 |
| Arp 299 | 46.8 ± 3.3 (a) | 688 ± 60 | 4470 ± 400 (k) | 41.52 ± 0.12 | 23.25 ± 0.07 | 24.07 ± 0.07 |
| NGC 4945 | 3.72 ± 0.27 (a) | 7953.52 ± 133 | * | 40.27 ± 0.07 | 22.12 ± 0.06 | * |
| Circinus | 4.21 ± 0.70 (a) | 1732.79 ± 218 | * | 40.15 ± 0.16 | 21.56 ± 0.15 | * |
| Arp 220 | 80.9 ± 5.7 (a) | 332 ± 3 | 315 ± 59 (l) | 42.41 ± 0.08 | 23.41 ± 0.06 | 23.39 ± 0.10 |
| Milky Way | * | * | * | 38.91 ± 0.13 (l) | 21.28 ± 0.14 (l) | * |
References. (a) Kornecki et al. (2020) and references therein. (b) Dennison et al. (1975). (c) Loiseau et al. (1987). (d) Hughes et al. (2007). (e)Computed from F1.4 GHz. (f) Strong et al. (2010). (g) Durdin & Terzian (1972). (h) Kapińska et al. (2017). (i) For et al. (2018). (j) Chyży et al. (2018). (k) Cox et al. (1988). (l) Varenius et al. (2016). (m) Israel et al. (1992). (n) Kuehr et al. (1981). (o) Hales et al. (1991).
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