Top panel: so-called perihelion outburst (jet 8 in Table A.1) from two color sequences acquired on 12 August 2015 starting at 17h20 and 17h50. Bottom right panel: RGB color image (composed from filters centered at 882, 649,and 480 nm), and image of the selected ROI. The color difference at the left edge of the outburst in the RGB image arises because the comet rotated between the three exposures. Bottom left panel: spectrophotometry of the nucleus and along the collimated component of the outburst.