Extended Data Fig. 1: Spatial distribution of the emission of key lines.
From: OH as a probe of the warm-water cycle in planet-forming disks
(Top Left) d203-506 image from the NIRCam F212N filter (in MJy sr−1), (Top Right) NIRSpec integrated intensity map of the OH line at 2.934 μm (in erg cm−2s−1sr−1), (Bottom Left) MIRI-MRS integrated intensity map of the OH line at 9.791 μm (in erg cm−2s−1sr−1), (Bottom Right) integrated intensity map of the [OI] line at 0.63 μm obtained from the Hubble Space Telescope (HST) (in counts s−1)28. The NIRSpec H2 1-0 S(1) intensity map is shown in white contours (at 7 × 10−4, 2 × 10−3 erg cm−2s−1sr−1).
