The MeerKAT Absorption Line Survey (MALS) data release 3: Cold atomic gas associated with the Milky Way

Open Access

Fig. B.1

Left: Distributions of line width (σ) of injected absorption lines and detections for peak and integrated S/N cutoffs adopted for the MALS sample. In general, for absorption features with single Gaussian component fits, integrated S/N = peak S/N × $\sqrt{\frac{Line FWHM}{Spectral resolution}}$ $\[\sqrt{\frac{\text {Line FWHM}}{\text {Spectral resolution}}}\]$ . Right: Distributions of line width of 2986 MALS absorbers fit with single Gaussian components.

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