Fig. 2.

g-band imaging of SN 2016hnk and its host galaxy, before (left) and after (middle) subtracting the host galaxy template using hotpants integration in SNOOPY. This example shows how the subtracted image is clean enough to perform PSF fitting, as shown in the right panel where the SN PSF has been removed. A small residual of the galaxy core is shown on the middle and right panels (white blob), however it does not affect SN PSF fitting.
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