Fig. A.1
SEDs of GASPS Herbig Ae/Be stars. PACS fluxes reported in this work can be identified with red triangles. Red arrows are 3σ upper limits. Blue circles correspond to literature data from Table A.2. The solid dark red line shows IUE spectrum and purple line for the Spitzer/IRS spectrum. The solid black line is the PHOENIX/Gaia model fitted to the stellar photospheric emission.
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