&gt;  I wonder if this says more about our sensor technologies than how the galaxy actually looks (the visible, infrared and microwave images look far richer than the others).<p>There are definite effects from technology. The radio and far-infrared observations are at much lower angular resolution than the optical and near-infrared, for example. So there&#x27;s less spatial detail in those. Also, some surveys have been carried out in more than one filter&#x2F;color (e.g., optical, near-infrared) and so the optical image shows some information about the color of objects in the optical. In contrast, the radio image appears to be a single frequency, and so doesn&#x27;t contain that information for the radio sources.<p>However, there is a lot of information there about the galaxy. The distribution of sources, for example – you can see the well-defined disk of the galaxy in all bands. The dust lanes corresponding to gas clouds are apparent in the optical as the dark patches. You can also see that there are some sources which emit brightly in X-rays, but are not seen in the other images. So that tells you about the types of objects in the galaxy.<p>So, despite the fact that the technology affects the images, I would not say that the map says less about the galaxy than about the technology.