The Cygnus Allscale Survey of Chemistry and Dynamical Environments: CASCADE - Overview and first results toward DR20 from the Max Planck IRAM Observatory program (MIOP)

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Fig. A.1

Integrated intensities for the species marked in each panel. The integration ranges are always from −7 to 3 km s⁻¹. Only for HCN and H¹³CN were broader integration ranges from −14 to 8 km s⁻¹ used to cover all hyperfine structures of the line. The data were clipped below the 4σ level for each species (Table 1).

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