Spectral energy distributions of the objects BRAN 76 (top left), EX Lupi (top right), Haro 5a IRS (middle left), HH 354 IRS (middle right), HH 381 IRS (bottom left), and Parsamian 21 (bottom right) including PACS spectra and photometry data (turquoise line + blue dots at 70, 100, and 160 μm), SPIRE high-resolution spectra (dark blue and red lines), and SPIRE photometry (black dots at 250, 350, and 500 μm) combined with spectra from Spitzer (lines in other colors below 50 μm) and photometry from other sources (diamonds; color-coded by source).