Image Details
Caption: Figure 1.
Final processed images of the TW Hya protoplanetary disk. Panel (a) shows the result in the F200W filter, and panel (b) shows the F444W result. Both left images are the product of HPFRDI, which subtracts the stellar PSF. The right images undergo a further deconvolution process with winnie, utilizing 200 iterations (for F200W) and 129 iterations (for F444W) of the Richardson–Lucy algorithm. The images resolve the nearly face-on disk structure.
© 2026. The Author(s). Published by the American Astronomical Society.