Open Access

Table D.1

LaccLline linear fit parameters.


Line λ0 [nm] a b c.f. σ Npoints Comments

H3(Hα) 656.28 1.27±0.08 2.37±0.19 0.9 0.11±0.02 59
H4(Hβ) 486.13 1.17±0.06 2.95±0.18 0.9 0.08±0.02 58
H5(Hγ) 434.05 1.14±0.06 3.01±0.18 0.9 0.08±0.02 54
H6(Hδ) 410.17 1.13±0.06 3.10±0.18 1.0 0.07±0.02 54
H7(Hϵ) 397.01 1.18±0.06 3.08±0.19 0.9 0.09±0.02 60 blended
H8 388.90 1.14±0.06 3.27±0.20 0.9 0.08±0.02 56
H9 383.54 1.09±0.05 3.15±0.18 0.9 0.08±0.02 56
H10 379.79 1.09±0.05 3.29±0.19 0.9 0.08±0.02 56
H11 377.06 1.13±0.07 3.52±0.24 0.9 0.11±0.02 58
H12 375.02 1.06±0.06 3.40±0.20 0.9 0.09±0.02 53
H13 373.44 1.01±0.06 3.27±0.21 0.9 0.11±0.02 51
H14 372.19 0.98±0.06 3.27±0.21 0.9 0.12±0.03 51
H15 371.20 1.08±0.13 3.68±0.49 0.8 0.49±0.10 58
Pa5(Paβ) 1281.81 1.20±0.09 3.68±0.31 0.9 0.14±0.03 51
Pa6(Paγ) 1093.81 1.20±0.08 3.80±0.28 0.9 0.12±0.02 56
Pa7(Paδ) 1004.94 1.38±0.11 4.71±0.40 0.9 0.11±0.03 50
Pa8 954.60 1.22±0.11 4.34±0.41 0.9 0.14±0.03 48
Pa9 922.90 1.25±0.09 4.55±0.35 0.9 0.13±0.03 56
Pa10 901.49 1.46±0.13 5.70±0.53 0.9 0.13±0.03 49
Br7(Brγ) 2166.12 1.08±0.11 4.18±0.46 0.9 0.24±0.06 45
HeI 402.62 1.15±0.11 4.22±0.43 0.8 0.28±0.06 61
HeI 447.15 1.17±0.07 4.24±0.29 0.9 0.10±0.02 55
HeI 471.31 1.28±0.13 5.43±0.56 0.8 0.20±0.05 53
HeIFeI 492.19 1.05±0.07 3.85±0.28 0.9 0.13±0.03 43 blended
HeI 501.57 0.88±0.07 3.09±0.29 0.9 0.23±0.06 38
HeI 587.56 1.19±0.07 4.01±0.25 0.9 0.08±0.02 57
HeI 667.82 1.47±0.09 6.01±0.39 0.9 0.06±0.01 43
HeI 706.52 1.33±0.08 5.46±0.35 0.9 0.06±0.02 48
HeII 468.58 1.21±0.11 4.91±0.49 0.9 0.18±0.04 49
CaII(K) 393.37 1.10±0.08 3.01±0.25 0.9 0.19±0.04 61
CaII(H) 396.85 1.18±0.06 3.09±0.19 0.9 0.09±0.02 60 blended
CaII 849.80 1.11±0.13 3.71±0.47 0.8 0.38±0.08 53
CaII 854.21 1.10±0.13 3.57±0.45 0.8 0.34±0.08 49
CaII 866.21 1.01±0.12 3.37±0.45 0.9 0.46±0.11 46
NaI 589.00 1.23±0.25 5.07±1.09 0.8 0.32±0.14 18
NaI 589.59 1.14±0.26 4.65±1.14 0.8 0.38±0.26 14
OI 777.31 1.24±0.12 5.02±0.51 0.9 0.19±0.05 43 blended
OI 844.64 1.49±0.15 5.49±0.58 0.9 0.12±0.03 41

Notes. We used Lacc as results drawn from the HST modelling of the HST-ULLYSES data and Lline obtained via a dereddening with AVHST$\[A_{V}^{H S T}\]$ as the observed flux of the accretion tracers detected in the PENELLOPE sample; λ0 is the central wavelength of the line; a and b coefficients are the best fit of Eq. D.1; c.f. stands for correlation factor between Lacc and Lline, σ is the spread of the distribution, and Npoints is the number of points for the fit over the total sample.

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