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Fig. 1
ROSAT RASS 30′ × 30′ image of G308.4–1.4 (0.1–2.4 keV) overlaid with the SUMSS image at 843 MHz (contour lines at 4, 8, 12, 16, and 25 mJy). The half-power beam-width of the telescope is 43′′. The RASS image is binned with 0.75′ per pixel and smoothed by a Gaussian kernel of σ ≈ 2′.
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