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Fig. 3

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Averaged MIDI flux (thin full lines) for different visual phases and overplotted ISO/SWS flux (thick black full line) of SV Psc in the N-band. Error bars denote the standard deviation of all observed fluxes for the respective night and telescope. The ISO SWS spectrum was observed in 1998 (i.e. 33 cycles before the first MIDI observations).

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