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The HI Mass Function of Star-forming Galaxies at z ∼ 0.35

  • Authors: Apurba Bera, Nissim Kanekar, Jayaram N. Chengalur, Jasjeet S. Bagla

Apurba Bera et al 2022 The Astrophysical Journal Letters 940 .

  • Provider: AAS Journals

Caption: Figure 2.

The M H IM B relation for blue galaxies at z ∼ 0.35: The solid blue circles show our estimates of ﹩\langle \mathrm{log}({{\rm{M}}}_{{\rm{H}}\,{\rm\small{I}}})\rangle ﹩ values in blue galaxies in the three M B bins at z ≈ 0.35 plotted against the median M B values. The error bars are estimated by jackknife resampling. The horizontal error bars show the bin widths. The solid black line shows the best-fit M H IM B scaling relation at z ≈ 0.35, while the blue shaded region shows the 68% confidence interval around the scaling relation. The red dashed line indicates the M H IM B relation at z ≈ 0 (Dénes et al. 2014).

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