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Fig. 22.

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HST image of the host galaxy of SN 2020qlb, corresponding to a rest-frame wavelength of 2900 Å, and taken at a phase of +386 days past the g-band peak. The host galaxy appears to have two knots of emission, with the supernova located at the northern knot. The apparent point source could include supernova emission, or be a star-forming region in the host galaxy; a template image would be needed to tell the two apart. The source visible in the bottom left of the image is caused by a cosmic ray.

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