SN 2020pvb: A Type IIn-P supernova with a precursor outburst

Open Access

Fig. 11.

$2 \overset{″}{.} 3 \times 2 \overset{″}{.} 3$ $2{{\overset{\prime\prime}{.}}}3 \times 2{{\overset{\prime\prime}{.}}}3$ cutouts from the 2017 HST+ACS/WFC image of the SN 2020pvb site. The dashed circles are centred at the SN 2020pvb position and indicate 0 $\overset{″}{.}$ ${{\overset{\prime\prime}{.}}}$ 11 and 0 $\overset{″}{.}$ ${{\overset{\prime\prime}{.}}}$ 55 (5σ significance) positional uncertainties based on the RMS uncertainty obtained from the astrometry. Red points are the likely stellar sources detected by DOLPHOT at these areas.

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