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Table 2

Molecular data for the pure rotational transitions along with the integrated fluxes of our model (Figure 5) and observations.

Transition Line center (μm) Eup (K) gu Integrated flux (10−16 erg cm−2s−1)
Model (i = 90°) Tau 042021 (total) SY Cha (0.5-2.0″)
S(1) 17.0348 1015.084 21 7.2 16 4.8
S(2) 12.2786 1681.639 9 2.8 7.8 5.5
S(3) 9.66491 2503.744 33 6.1 17 25
S(4) 8.02504 3474.498 13 1.3 5.6 9.1
S(5) 6.90951 4586.059 45 1.9 11 25
S(6) 6.10856 5829.842 17 0.30 1.9 8.3
S(7) 5.51118 7196.708 57 0.37 3.8 17
S(8) 5.05312 8677.149 21 0.053 1.1 5.5
S(9) 4.69461 10261.45 69 0.065 4.5

Notes. The Tau 042021 fluxes represent the total flux from both the western and eastern lobes of the disk. The data are primarily taken from Table 1 of Arulanantham et al. (2024), with the S(9) flux adopted from Pascucci et al. (2025). Note that the spatial integration areas are larger in our model than in the Tau 042021 observations, so direct quantitative comparisons should be made with caution (see Section 4.4.1 for details). The SY Cha fluxes are adopted from Schwarz et al. (2025a), measured with a radius aperture of 0.5-2.0" (note that d = 180.7 pc).

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