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Table 2.

Results of the model fit of the SED in the high mode for J1544 (this work) and J1023 (Baglio et al. 2023).

Component Parameter Posterior Prior bounds


J1544 J1023( * ) J1544 J1023( * )
Irradiated star T* (K) 4115 98 + 103 $ 4115^{+103}_{-98} $ 6141 30 + 33 $ 6141^{+33}_{-30} $ 𝒩(4100, 100)( ⋆ ) 𝒩(6128, 33)
Log [Lirr/1 erg/s] 33.7 ± 0.1 33.8( † ) 𝒰(30, 40)
Accretion disk Log [rin, opt/UV/1 cm] 9.09 ± 0.2 9.49 ± 0.02 𝒰(7, 12) 𝒰(7, 12)
Boundary emission Log [νsync/1 Hz] 15 . 2 0.1 + 0.4 $ 15.2^{+0.4}_{-0.1} $ 14 . 3 0.3 + 0.4 $ 14.3^{+0.4}_{-0.3} $ 𝒰(10, 16) 𝒰(12, 16)
αsync −0.723 ± 0.003 −0.61 ± 0.01 𝒰(0.4, 1.0) 𝒰(−0.9, −0.4)
Log [Fsync/1 mJy] 1 . 6 0.3 + 0.1 $ -1.6^{+0.1}_{-0.3} $ 1 . 1 0.3 + 0.2 $ -1.1_{-0.3}^{+0.2} $ 𝒰(−5, 5) 𝒰(−3, 2)
Compact jet Log [νbreak/1 Hz] 13.4 ± 0.3 𝒰(10, 14)
α1 0.18 ± 0.06 𝒩(0.2, 0.2)
α2 −0.78 ± 0.04 𝒩(−0.7, 0.2)
Log [F0/1 mJy] −0.6 ± 0.2 𝒰(−2, 0)

Notes. We report the median values of the posterior distributions for the model parameters, along with their lower and upper uncertainties, for J1023 (from Baglio et al. (2023) and indicated as ( * ), including prior assumptions from references therein) and J1544 (this work). These uncertainties correspond to the 15.9th and 84.1st percentiles of the posterior distributions for each parameter. The final column provides the prior bounds applied to all parameters, where 𝒩(μ, σ) represents a normal distribution with a mean μ and variance σ2, and 𝒰(a, b) denotes a uniform distribution in the (a, b) interval. ( † ) Fixed at 6.5 × 1033 erg/s (Baglio et al. 2023). ( ⋆ ) From Britt et al. (2017); see Sect. 4 for a detailed discussion on the irradiation component.

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