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Fig. 1


HD 142527 ISO LWS spectra before and after splicing. In general the difference before and after splicing is small. We indicate the data from detectors 7 and 9, which were shifted down by −6 and −14 Jy, respectively, to form a continuous spectrum. The overall shape from 45 to 200μm of the dust emission is unaffected by the splicing we applied. The only line emission that is significantly detected is the [Cii] at 158μm.

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