ExoplaNeT accRetion mOnitoring sPectroscopic surveY (ENTROPY) - III. Optical He I line profiles of the accreting super Jupiter Delorme 1 (AB)b

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Table F.1

L_acc and Ṁ_acc measured from Delorme 1 (AB)b using different parameters.

Epoch	Measured from	log(L_acc/L_⊙)	Ṁ_acc(M_⊙ yr⁻¹)
UVES	UV excess	$- {5.3}_{- 0.4}^{+ 0.5}$ $Mathematical equation: $-5.3^{+0.5}_{-0.4}$$	1 - 3 × 10⁻¹²
UVES	He I (FAM25)	$- {4.9}_{- 0.3}^{+ 0.3}$ $Mathematical equation: $-4.9^{+0.3}_{-0.3}$$	7.4 × 10⁻¹²
UVES	Hα (FAM25)	$- {5.5}_{- 0.2}^{+ 0.4}$ $Mathematical equation: $-5.5^{+0.4}_{-0.2}$$	1.4 × 10⁻¹²
UVES	Hα (AMI21)	$- {4.3}_{- 0.2}^{+ 0.3}$ $Mathematical equation: $-4.3^{+0.3}_{-0.2}$$	2.6 × 10⁻¹¹
MUSE	Hα (FAM25)	$- {6.6}_{- 0.2}^{+ 0.4}$ $Mathematical equation: $-6.6^{+0.4}_{-0.2}$$	1.3 × 10⁻¹³

Notes. FAM25 and AMI21 denotes L_line-L_acc scaling relations from Fiorellino et al. (2025) and Aoyama et al. (2021) respectively. The uncertainties indicated on the L_acc measurements are based on the lowest and highest values over the observations epochs.

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