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Alex Dvornikov edited figures/iPTF15dgq_Light_Curves/caption.tex
over 8 years ago
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Replace this text with your caption Despite the jaggedness (likely due to poor seeing on certain nights) we did not resort to fixed size aperture photometry. The dynamic FHWM method seemed fruitful for most of the nights. Judging from the finding charts, neither supernova is heavily polluted by a background galaxy or a nearby star.
