Extended Data Table 1 Absorption line measurements for the z = 2.54290 DLA

From: Resolving the H i in damped Lyman α systems that power star formation

  1. aAperture name as denoted in Fig. 1. bMeasured H i column densities from Voigt profile fitting. Errors are ±1σ uncertainties on column densities. cRest-frame equivalent widths of different metal absorption lines in units of mÅ. Errors are ±1σ uncertainties on equivalent widths. The < signs denote 2σ non-detection limits.
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