Extended Data Table 1 Voigt profile model parameters for the Magellanic CGM

From: Observations of a Magellanic Corona

  1. Best-fit model parameters for C IV and Si IV for components associated with Magellanic CGM with vLSR > 150 km s−1. For each sightline, the LMC impact parameter ρ, centroid velocity v, Doppler parameter (linewidth; b), column density log10(N/cm−2) and photoionized fraction fPI (fPI = NCloudy/NObs) for both ions are given. Components with fPI ≤ 0.1 are considered as not photoionized and shown in Fig. 3. Linewidths from data with low S/N ratio spectra or that are fixed in the fitting process do not show errors. Uncertainties in this table correspond to 1σ standard deviations. Further fit results for all ions and sightlines can be viewed at https://github.com/Deech08/HST_MagellanicCorona.
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