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Table 2

Results for the analyzed flux maps.

Resolution Mass Type FVIS(FVISstar /FVIS)${{\rm{F}}_{{\rm{VIS}}}}\left( {{\rm{F}}_{{\rm{VIS}}}^{{\rm{star}}}/{{\rm{F}}_{{\rm{VIS}}}}} \right)$ FNIR FNIRstar${\rm{F}}_{{\rm{NIR}}}^{{\rm{star}}}$ FNIR dust, scattered ${\rm{F}}_{{\rm{NIR}}}^{{\rm{dust, scattered}}}$ FNIR dust, direct${\rm{F}}_{{\rm{NIR}}}^{{\rm{dust, direct}}}$ Fsubmm(Fdust,direct /Fsubmm)
N1 300 M RT 0.33 Jy (99.94%) 0.52 Jy 0.36 Jy 0.02 Jy 0.14Jy 1.00 Jy (>99.99%)
N1 300 M RHD 0.34 Jy (99.99%) 0.79 Jy 0.36 Jy 0.06Jy 0.37 Jy 0.87 Jy (99.99%)
N1 10 M RT 0.33 Jy (99.94%) 0.52 Jy 0.36 Jy 0.02 Jy 0.14Jy 1.09 Jy (>99.99%)
N1 10 M RHD 0.34Jy(99.99%) 0.79 Jy 0.36 Jy 0.06Jy 0.37 Jy 1.02 Jy (>99.99%)

N3 300 M RT 0.34 Jy (99.94%) 0.55 Jy 0.36 Jy 0.02 Jy 0.17Jy 1.03 Jy (>99.99%)
N3 300 M RHD 0.34 Jy (99.98%) 0.87 Jy 0.36Jy 0.05 Jy 0.45 Jy 0.98 Jy (>99.99%)
N3 10 M RT 0.34 Jy (99.94%) 0.55 Jy 0.36Jy 0.02 Jy 0.17Jy 1.08 Jy (>99.99%)
N3 10 M RHD 0.34Jy(99.98%) 0.87 Jy 0.36Jy 0.05 Jy 0.45 Jy 1.08 Jy (>99.99%)

Notes. Model parameters (resolution, planetary mass, and simulation type) are listed in the first three columns. Total flux values for the VIS (FVIS), NIR (FNIR), and submm (Fsubmm) wavelength ranges are shown in the fourth, fifth, and ninth column, respectively. Bracketed values denote the contributions of the dominant flux sources to the total flux in percent. The flux value Fωs${\rm{F}}_\omega ^s$ corresponds to the simulated contribution of the source s (e.g., the star, scattered thermal emission from the dust, or direct unscattered thermal dust emission) to the total flux observed in the wavelength range ω. For the NIR, a complete breakdown of the contributions of three different sources to the total flux are presented in the sixth to eighth columns.

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