Extended Data Table 2 Voigt profile model parameters for O VI

From: Observations of a Magellanic Corona

  1. Best-fit model parameters for O VI for components associated with Magellanic CGM with vLSR > 150 km s−1. Linewidths without errors are shown when they are fixed in the fitting process. Further fit results for all ions and sightlines can be viewed at https://github.com/Deech08/HST_MagellanicCorona.
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