Table 3
Mass values of the host.
| M(r) [M⊙] | RAR 1 (m = 56 keV) | RAR 2 (m = 56 keV) | RAR 3 (m = 20 keV) | Burkert |
|---|---|---|---|---|
| M(rc) | 3.5 × 106 | 3.5 × 106 | 3.5 × 106 | – |
| M(r = 12 kpc) | 3 × 1010 | 7 × 1010 | 5 × 1010 | 5 × 1010 |
| M(r = 40 kpc) | 2.2 × 1011 | 2.5 × 1011 | 2.2 × 1011 | 2.2 × 1011 |
| M(r = 80 kpc) | 2.4 × 1011 | 2.7 × 1011 | 4 × 1011 | 4 × 1011 |
Notes. Accumulated DM mass values used to fit the RAR 2, RAR 3, and Burkert halos of the hosts involved in the spray algorithm. The values are taken from Gibbons et al. (2014), as is detailed in Sect. 3. rc is the core radius of the fermionic models. While both models RAR 1 and RAR 2 develop a polytropic halo tail with a dense DM-core (on miliparsec scales) alternative to the central BH, the model RAR 3 develops a power-law-like halo trend (similar to Burkert).
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