English: From "Polarised radio pulsations from a new T-dwarf binary"
Figure 3:
Contour plots of one typical individual exposure for each filter in which we obtained infrared data. Contours are drawn in logarithmic intervals from the peak flux down to 10% of the peak flux in each image. The images are all 15 across with north being up. In 2015, despite the AO correction deteriorating from 009 in the CH4s band to 013 in the J band, the binary was still well resolved. We used the more precise differential magnitudes from the higher-quality, and fully contemporaneous 2022 images in our analysis.
I did cut the image with Photoshop Elements to only show the 2022 J-band image.
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