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Table 3.

Simulation results for different molecular cloud mass distributions.

α Itot IQR
[Jy km s−1] [Jy km s−1] [Jy km s−1]
−1.50 1.91 × 10−3 7.04 × 101 5.91 × 10−3
−1.64 1.86 × 10−3 7.02 × 101 5.85 × 10−3
−2.00 1.72 × 10−3 6.61 × 101 5.40 × 10−3
−2.90 1.51 × 10−3 5.91 × 101 4.68 × 10−3

Notes. Results from running ten simulations per model configuration: α – power-law slope of the molecular cloud mass distribution, – median flux, (Itot) – total galactic emission, IQR – midspread.

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