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Table 3

Atmospheric parameters derived from the measured IQ at different wavelengths from MUSE data cubes.

DIMM-seeing along MUSE direction Negligible dome-seeing Non-negligible dome-seeing

MUSE Field (1) εMUSE (2) ϵ0b$\[\epsilon_0^b\]$ (3) 0b$\[\mathcal{L}_0^b\]$ (4) εdome (5) ϵ0b$\[\epsilon_0^b\]$ (6) 0b$\[\mathcal{L}_0^b\]$ (7) εdome (8) γ (9)
HD 90177a 0.57 0.79 20.3 ± 1.5 0.00 0.76 12.6 ± 1.3 0.25 3.81 ± 0.11
HD 90177b 0.45 0.76 20.5 ± 1.6 0.00 0.69 16.1 ± 1.9 0.28 3.61 ± 0.06
HD 90177c 0.58 0.81 16.3 ± 1.1 0.00 0.76 10.8 ± 1.2 0.28 3.72 ± 0.09
HD 90177d 0.57 0.70 28.1 ± 2.6 0.00 0.69 9.3 ± 0.9 0.29 3.97 ± 0.04
OGLEII 0.53 0.93 15.9 ± 1.1 0.00 0.84 32.6 ± 6.6 0.17 3.03 ± 0.05

Notes. Columns correspond to: (1) MUSE observed field. (2) ε0 (in arcsec) along the MUSE observing direction estimated from the DIMM value corrected from the Nasmyth platform altitude respecting DIMM and airmass. (3) and (4) Combination of ε0 and 0$\[\mathcal{L}_0\]$ values minimizing residuals when comparing the predicted εLE using Eq. (5) with these values with the measured IQ at any wavelength, assuming a negligible dome turbulence contribution (5). (6) and (7) Combination of ε0 and 0$\[\mathcal{L}_0\]$ values minimizing residuals when comparing the predicted εLE using Eq. (5) with the measured IQMUSE> at any wavelength, considering the contribution of the εdome. Uncertainties for Cols. (3) and (6) are consistently 0.01 arcsec, corresponding to the ε0 steps in the iterative process, with units in arcsec. Columns (4) and (7) are in units of meters. (8) Estimated turbulence contribution (in arcseconds) of the dome enclosure at the reference wavelength of 7000 Å (Racine et al. 1991). (9) Power-law index for the wavelength dependence of the εdome.

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