Comparison of the SPARTA and Eureka! reductions for the NIRCam spectrum from Hu et al. (2024). The dark grey data points represent SPARTA, while the light brown error bars are for Eureka!. Note that the SPARTA spectrum is lower resolution (21 points, versus 30 for Eureka!), which naturally results in lower χ² values. The black spectrum is the total emission, with major absorbers highlighted in colour. Also shown in red is the low-flux Spitzer measurement from Demory et al. (2016b).