Online Material
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Figure 1: Baseline-subtracted H I profiles of the 162 detections in the Crux/GA region. The vertical axis gives the flux density in mJy, the horizontal axis the velocity range (optical convention), generally centred on the velocity of the galaxy and displaying a width of 1600 km s-1. All spectra are baseline-subtracted and generally Hanning-smoothed. The identifications are given within the panels. Question marks indicate uncertain identifications, stars denote a detection not at the centre of the beam. |
| Open with DEXTER | |
![\begin{figure}
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Figure 1: continued. |
| Open with DEXTER | |
![\begin{figure}
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Figure 1: continued. |
| Open with DEXTER | |
![\begin{figure}
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Figure 1: continued. |
| Open with DEXTER | |
![\begin{figure}
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Figure 1: continued. |
| Open with DEXTER | |