Eclipse mapping study of the eclipsing binary KIC 3858884 with hybrid delta Sct/gamma Dor component

Supplementary material of the paper with the same title accepted for publishing by Astronomy & Astrophysics. Table A.1.: First 55 detected frequencies with the highest amplitude. The associated frequencies in both units of orbital frequencies and c/d, the amplitude and phases are presented. In the last column the possible frequency combination is indicated as well. Fig. A.1.: Synthetic modulations of considered ($\ell$,$m$) modes during the secondary eclipse. All modes were modelled with the same frequency and out of eclipse amplitude. The associated non-negative ($\ell$,$m$)-s are labelled with the proper colour in the middles of the panels. The dashed pairs of non-zero modes are the negative $m$ sibling of the same mode. They are grouped as a 'families' according their resemblance to each other. Fig. A.2.: Fourier-spectra of all modelled, non-negative ($\ell$,$m$) modes calculated by \texttt{SigSpec}. The first four row presents all modes which are more distinguishable pairs from the different families shown in Fig.A.1. In the last row illustrates the hidden modes with the largest amplitude. The mode numbers are labelled in right top corner of each panel, the colours are meant to assistance to compare with the associated 'family member' in Fig.A.1. Note that the amplitudes are showed on a square-root scale for a better visibility of the side peak forests. Fig.B.1.: Result of YLMCMC, aligned configuration. For a more detailed discussion, please refer to the relevant article.