Testing analytical methods to derive the cosmic-ray ionisation rate in cold regions via synthetic observations

Open Access

Fig. 8

Ratio between ζ₂ retrieved in each run (x-axis labels), and the actual value $ζ_{2}^{s}$ $\zeta _2^s$ . The ratios are median computed in each map, in the same regions used to produce the histograms of Fig. 1. The shaded areas show a variation of a factor of 2 (darker shade) or 3 (lighter shade). The dashed line represents where the ratio is equal to 1. The error bars are 3σ median uncertainties.

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