The GROND gamma-ray burst sample - I. Overview and statistics

Open Access

Fig. A.10.

Swift/UVOT white (left) and GROND g′ image (right) of GRB 140619A. The ≈3 mag fading confirms the afterglow nature of the UVOT detection, and the GROND detection two months later is likely the GRB host galaxy. The circle (radius 1 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 4) is to guide the eye; the Swift/XRT error circle (1 $\overset{″}{.}$ $\overset{\prime \prime }{.}$ 7) is omitted for better legibility.

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