Extended Data Table 2 Emission line fluxes and limits

From: Confirmation and refutation of very luminous galaxies in the early Universe

  1. Integrated flux and limits for the main emission lines detected in the nine spectroscopically confirmed sources presented in this work, sorted by decreasing redshift as in Extended Data Table 1. All values are in units of 10−20 erg s−1 cm−2 and all uncertainties listed are 68% confidence intervals. Upper limits are presented at 3σ. The fluxes presented in this table have been measured after rescaling the spectra to the NIRCam photometry but note that small uncertainties due to imperfect photometric calibration and wavelength dependant slit losses may still affect these measurements and so they should be taken with caution.