Image Details
Caption: Figure A1.
Images of the selected sources (Table 1) produced from the self-calibrated data (Section 3.2) at the frequency range of 286–294 GHz (Table 2). Each panel shows the 8″ wide square region centering at the peak of the target source. The DoAr 24E panel covers the binary components DoAr 24Ea and DoAr 24Eb. Contours start at 3σ, with 3σ intervals.
© 2026. The Author(s). Published by the American Astronomical Society.