Image Details
Caption: Figure 6.
(left) NIRCam subarray PCA reduction at F444W showing the source S1 at ∼2 o’clock. (Center and right) MIRI observations optimized for point-source detection identifies the same source at F1550 and F2550W, strongly suggesting this object is extragalactic in nature (K. Y. L. Su et al. 2024, in preparation). In all three images intensity units are MJy sr−1.
© 2024. The Author(s). Published by the American Astronomical Society.