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Fig. 5.
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X-ray image of NGC 4303 obtained with Chandra, observed in August 2001. None of the historical SNe have an associated source in X-ray, but both SNR 4303-46 and SNR 4303-20 are detected. SNR 4303-20 is considerably dimmer compared to SNR 4303-46, while SNR 4303-37 has very faint detection.
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