Table C.1
Mass accretion rates obtained from the MUSE spectra in Sect. 4.5, with AV taken to be 1.26 mag.
| Line | λ (Å) |
A | B | Lline (10-5 L⊙) |
ΔLline – |
Lacc (10−3 L⊙) |
ΔLacc | Ṁacc (10−8 M⊙ yr−1) |
Δ Ṁacc – |
Obsc. |
|---|---|---|---|---|---|---|---|---|---|---|
| Hβ | 4861.33 | 1.14 ±0.04 | 2.59 ±0.16 | 22.0 | 1.1 | 26.4 | 6.38 | 43.9 | 10.6 | 28 |
| He I λ14922 | 4921.93 | 0.97 ± 0.04 | 3.08 ±0.24 | 0.86 | 0.04 | 14.6 | 3.79 | 24.3 | 6.32 | 42 |
| [O I] 6300 | 6300.304 | 1.33 ±0.14 | 5.37 ±o.62 | 25.6 | 1.28 | 3.92 × 103 | 0.93 × 103 | 19.1 | 4.55 | − |
| Hα | 6562.8 | 1.13 ±0.05 | 1.74 ±0.19 | 74.5 | 3.72 | 16.0 | 3.83 | 26.7 | 6.38 | 39 |
| He I λ16678 | 6678.2 | 1.25 ±0.06 | 4.7 ± 0.33 | 0.30 | 0.015 | 6.32 | 1.59 | 10.5 | 2.65 | 73 |
| He I λ17065 | 7065.2 | 1.18 ±0.05 | 4.47 ± o.29 | 0.67 | 0.03 | 23.3 | 5.86 | 38.8 | 9.76 | 30 |
| O I λ18446 | 8446.36 | 1.08 ±0.12 | 3.46 ±o.62 | 0.8 | 0.04 | 9.04 | 2.3 | 15.0 | 3.83 | 57 |
| Ca II λ18498 | 8498.0 | 0.99 ± 0.05 | 2.6 ±0.29 | 2.34 | 0.12 | 10.4 | 2.64 | 17.3 | 4.39 | 52 |
| Ca II 8542 | 8542.09 | 0.97 ± 0.06 | 2.43 ±o.29 | 2.73 | 0.14 | 10.1 | 2.56 | 16.7 | 4.26 | 53 |
| Ca II λ18662 | 8662.14 | 0.93 ± 0.06 | 2.30 ±0.3 | 2.17 | 0.11 | 9.17 | 2.36 | 15.3 | 3.93 | 57 |
Notes. Emission line luminosities (Lline), accretion luminosities (Lacc), mass accretion rates (Macc) and corresponding uncertainties (ΔLline, ΔLacc, and ΔMacc, respectively) are listed. Mass accretion rates obtained from permitted lines are quoted after correction using the obscuration factors in the last column. The coefficients A and B are those obtained by Alcalá et al. (2014), except in the case of the [O I]λ6300 line where we use updated coefficients for the high-velocity jet from Nisini et al. (2018).
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