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Fig. 16.

image

Application of getsf to the XMM-Newtonλ ≈ 0.0024 μm image (7″ resolution) of the supernova remnant RX J1713.7−3946, adopting {X|Y}λ = {15, 25}″. The top row shows the original image ℐλ and the backgrounds ℬλ{X|Y} of sources and filaments. The middle row shows the component 𝒮λ, the footprint ellipses of 41 acceptably good sources on 𝒮λD (red squares mark the spurious peaks), and the component ℱλD with 13 non-branching skeletons 𝒦k2 corresponding to the scales Sk ≈ 40″. The bottom row shows the standard deviations 𝒰λ in the regularized component 𝒮λR, the flattening image 𝒬λ, and the standard deviations in the flattened component . Intensities (in photons cm−2 s−1) are limited in range with square-root color mapping, except for 𝒬λ, which is shown with linear mapping.

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