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Fig. B.1.


Spectral energy distributions of GCC sources 1446 to 1475. Blue diamonds are 2MASS J, H, and Ks fluxes from the 2MASS PSC. Green upwards-pointing triangles are Spitzer 3.6, 4.5, 5.8, 8.0, and 24 μm fluxes from the YSO catalogue of Renaud et al. (2013). Green downwards-pointing triangles are WISE 3.4, 4.6, 12, and 22 μm fluxes from our photometry measurements. Orange diamonds are AKARI 9, 18, 65, 90, 140, and 160 μm fluxes from the AKARI MIR and FIR point source catalogues. Red squares show the fluxes of PACS 100 and 160 μm from our photometry measurements. Black circles are fluxes of PACS 160 and SPIRE 250, 350, and 500 μm from the GCC catalogue of compact sources. For the fluxes selected from public point source catalogues, only the source nearest to the GCC source centre was considered. Error bars show the flux uncertainties, but can be smaller than the marker size. The source number in the GCC catalogue is indicated in the top left corner of each frame, along with our evolutionary state classification (SL and PS stand for starless and protostellar, respectively, and the numbers 1 and 2 for candidate and confirmed classification, respectively). The Spitzer-based classification by Renaud et al. (2013) is shown in parentheses.

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