Fig. 1.
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Broadband (0.5–1.0 keV) (particle) background-subtracted, exposure-corrected X-ray image (linear scale) obtained by SRG/eROSITA in the S147 direction (3.7° × 3.7° in Galactic coordinates) after masking of point and mildly extended sources and smoothing with a Gaussian kernel with σ = 1′. This band maximizes the source-to-background ratio for the SNR emission. The cross marks the position of the pulsar PSR.
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