Extended Data Fig. 7: J160532 line fluxes compared to other disks.
From: A rich hydrocarbon chemistry and high C to O ratio in the inner disk around a very low-mass star
This figure presents a comparison of C2H2 versus H2O line flux scaled to 140 pc for a number of T Tauri disks observed with Spitzer and complied by ref. 60 and J160532 observed with JWST MIRI. The line fluxes for J160532 are consistently calculated by integrating the flux of the three water features at 17.12 μm, 17.22 μm, and 17.36 μm, and the C2H2 feature over a window between 13.65-13.72 μm as explained in ref. 60. Leftward (resp. downward) arrows represent upper limits on H2O (resp. C2H2) line flux.
