Data from "The 2023 Australian Total Solar Eclipse: Line Emission of Fe XIV, Fe X, and Fe XI out to 6 Solar Radii"

Narrowband imaging data of the corona collected during the 2023 Total Solar Eclipse on April 20 in Australia. These data contain observations of the ionic emission lines of Fe X (637.4 nm), Fe XI (789.2 nm), and Fe XIV (530.3 nm) as well as corresponding continuum observations of the K and F corona near each line. The line emission data have already had the continuum subtracted.The data are contained in seperate files for both Cartesian coordinates and polar coordinates. Each file contains two layers: the first being the scientific data product of integrated brightness (in mean solar disk brightness units), and the second is an estimate of the uncertainty of the observation. Additional metadata are included in the FITS headers of each file.These data have already appeared in Boe et al. 2026, ApJ, 997, 171. See that publication for further details.https://iopscience.iop.org/article/10.3847/1538-4357/ae2658