Dust populations from 30 to 1000 au in the debris disk of HD 120326 - Panchromatic view with VLT/SPHERE, ALMA, and HST/STIS

Open Access

Fig. 9

Reflectance spectrum of the inner belt of HD 120326. For each point, we derive the surface brightness of the disk (SB_disk) and the stellar flux (F_⋆) over a spectral range shown by the horizontal line around each point, and also by the colored areas (IFS) or the filter transmission (IRDIS) at the bottom.

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