Fig. 2.
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H I mass sensitivity for the MGCLS. Top: logarithm of the total H I mass sensitivity as a function of redshift for integration times between 3 h and 12 h (not all MGCLS datasets have the same usable on-source time for H I analysis). The shaded areas indicate the H I mass limits of the MGCLS data assuming a 5σ detection for a galaxy with line width ranging from 44 km s−1 to 300 km s−1. Bottom: column-density sensitivity versus angular resolution at z = 0.03 for different integration times present in the MGCLS. The horizontal axis scale is proportional to HPBW−2.
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