All Tables

Table 1: Least squares fits to the magnetic field strength B, the optical depth normalization coefficient ${\cal T}_{\rm norm}$ , the scattering probability $c_{\rm sc}$ , the temperature of the isothermal CN layer $T_{\rm eff}$ and cosine of the heliocentic angle $\mu$ in three considered regions of spectrum
Table 2: Line parameters used for the fitting procedure in the first spectral region (3865.9-3866.8 Å). The columns list the wavelength ( $\lambda$ ), the line identification (ID), the polarizability (W₂), the lifetime of the upper level ( $\tau _R$ ), the turbulent magnetic field strength at which the line polarization is reduced to 30% of its non-magnetic value neglecting elastic collision (B₃₀), the vibrational number which coincides for the upper and lower states (v), and the oscillator strength (f_vJS).
Table 3: Line parameters used for the fitting procedure in the second spectral region (in the (1,1) bandhead), with the same parameters as in Table 2.
Table 4: Line parameters used for the fitting procedure in the third spectral region (close to the (0,0) bandhead), with the same parameters as in Table 2.