Table 4.
Parameters derived from SED fitting for the host galaxies of transients in our sample.
| Galaxy |  |
Lstarburst |  |
 |
LPolar | Cov factor | AGN frac | θi | θo | CCSNe rate | SF rate | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1011 L⊙ | 1011 L⊙ | 1011 L⊙ | 1011 L⊙ | 109 L⊙ | (%) | (%) | (°) | (°) | (SN yr−1) | (M⊙ yr−1) | ||
| AT 2017gbl pre | 4.35 |
1.61 |
0.43 |
1.40 |
0.01 |
0.01 |
32.2 |
60.8 |
43.6 |
 |
 |
(1,4) |
| AT 2017gbl post | 4.35 |
1.61 |
0.43 |
1.40 |
3.8 |
– | 32 |
60.8 |
43.6 |
 |
 |
(1,4) |
| Arp 299-B AT1 pre | 1.30 |
0.98 |
– | 0.32 |
0.52 |
3 |
24 |
– | – | 0.33 | 56 | (2),(3) |
| Arp 299-B AT1 post | 1.37 |
0.99 |
– | 0.30 |
7.78 |
52 |
23 |
– | – | 0.33 | 56 | (2),(3) |
| AM 0702-601N | 7.3 |
1.76 |
0.93 |
4.3 |
35 |
16.2 |
59 |
64.2 |
54.0 |
0.37 |
28 |
(4) |
| IRAS F05189−2524 | 56 |
7.7 |
5.5 |
47 |
98 |
4.2 |
84 |
68 |
60.0 |
0.9 |
70 |
(5) |
| ESO 286-IG019 | 23 |
6.7 |
2.7 |
14 |
1.1 |
0.2 |
64 |
80.3 |
41.1 |
0.9 |
67 |
(4) |
Notes. Luminosity values are bolometric. 
and 
denote the AGN luminosity pre- and post-correction for the anisotropy of the emission from the AGN torus, and 
includes this correction. θi denotes the inclination of the AGN torus, and θo is the torus opening angle, with both angles measured from the pole. The star formation rate of the starburst is averaged over the last 50 Myr. Values for Arp 299-B AT1 are for the Arp 299-B region and not for the entire galaxy system.
References. (1) K20; (2) M18; (3) Mattila et al. (2012); (4) this work; (5) Efstathiou et al. (2022).
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