Showing four images of the K mag = 2 star β Doradus taken as part of Program 1023 (observations 32–35) in four filters at 5.6, 7.7, 10 and 12.8 µm. The star was moved across the detector using offsets in the APT in order not to overlap the images. The bright star quickly (in less than 1 group = 2.7 s) saturates the detector at its centre (seen in black in these images). The images are presented in calibrated flux units (MJy sr⁻¹), processed to level 2b in the pipeline. At 5.6 µm an “imprint” of the JWST mirrors can be seen behind the source which is a persistence from slewing across the Flens as discussed in Sect. 9.1.1.