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<!-- DOI: 10.1051/0004-6361/200912592 -->

<h2 class="sec">Online Material</h2>

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<td class="img-txt"><span class="bold">Figure 1:</span><p>
Baseline-subtracted H  <SMALL>I</SMALL>&nbsp;profiles of the 162&nbsp;detections in
the Crux/GA&nbsp;region. The vertical axis gives the flux density in&nbsp;mJy, the horizontal axis the velocity range (optical convention), generally centred on the velocity of the galaxy and displaying a width of 1600&nbsp;km&nbsp;s<sup>-1</sup>. 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.</p></td>
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