Constraints on the local interstellar magnetic field from non-thermal emission of SN1006

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Fig. 5

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Top panel: synthesized radio image at 1 GHz for our best-fit model (GRAD2 in Table 1, and quasi-parallel injection efficiency scenario, φ_B = 38° and φ_∇|B| = 15°), smoothed with a sigma of 2′. Bottom panel: radio map of SN1006 of Fig. 2, but smoothed with the same sigma as for the model image.

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