Exposing the plural nature of molecular clouds - Extracting filaments and the cosmic infrared background against the true scale-free interstellar medium

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Fig. 9

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Gaussian (left) and coherent (right) reconstructed column density maps following Eqs. (19) and (20); the correction factor C_δ has been multiplied to both maps, and the mean values of the initial map μ₀ has been distributed to both maps.

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