Image Details
Caption: Figure 6.
Left: unconvolved ABA-3 exozodi model coplanar with the α Cen AB binary. Center: the exozodi model in the left panel after PSF convolution (for the 2025 April observation orientation). Right: PSF-subtracted image showing the recovery of the ABA-3 exozodi model injected in the raw α Cen AB data set from the 2025 April observations. The regions of the image affected by the MIRI/4QPM transition boundaries at each roll are masked. The aperture that yielded the highest S/N (=21.3) detection for the injected disk is shown (see Paper II for details). All images are plotted on a common logarithmic color scale.
© 2025. The Author(s). Published by the American Astronomical Society.