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Fig. 1

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HD 207129 spectral energy distribution. Red data points are the PACS and SPIRE photometry, black data points are the ancillary data, including the Spitzer IRS spectrum. Error bars are 1 σ and include both calibration uncertainty (10% for 70/100 μm, 20% for 160 μm) and sky noise. Some error bars are smaller than the data point symbol. For wavelengths longer than  ~30 μm the solid line represents a disc model with a λ0 = 210   μm and β = 1, the dashed line represents a disc model with a λ0 = 63   μm and β = 2.7 and the dotted line represent the stellar photosphere.

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