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Table 2
Polynomial fits used to approximate the continuum of each spectral band and observation.
| Spectral band | ObsID | Wavelengths used for the polynomial fit [µm] | a0 [Jy] | a1 [Jy µm−1] | a2 [Jy µm−2] |
|---|---|---|---|---|---|
| B3 | 1342186573 | 58.95–59.25, 67.4–67.7 | 113815 | -967.280 | |
| B2 | 1342186574 | 76.7–77.0, 91.6–91.9 | 89631.3 | -580.734 | |
| Rl | 1342186573 | 103.4–103.7, 152.0–152.3, 181.7–182.0 | 83536.0 | -743.613 | 1.80825 |
| Rl | 1342186574 | 103.4–103.7, 152.0–152.3, 181.7–182.0 | 57321.8 | ^30.794 | 0.916970 |
Notes. Equation (2) gives the mathematical expression to calculate each polynomial using its coefficients listed here. We set a2 = 0 for the approximation of the continua in the spectral bands B3 and B2.
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