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Fig. 10


Spitzer 3.6 μm images of the field of SN 2005at. Observation on 2006 September 25 (a) shows a clear detection of a source at the location of SN 2005at, indicated with tick marks, ~1.6 yr from the explosion. Non-detection was obtained on 2012 May 25.7 (b), ~7.3 yr from the explosion. The panels are 1 × 1 arcmin2 subsections. Orientation is indicated in the second panel.

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