Figure 5.
An example of a radio source where the window centred on the host galaxy, shown as a rectangle, does not contain enough radio information to correctly identify the galaxy as the host. The background image is a 3.6 µm image from SWIRE. The contours show ATLAS radio data and start at 4σ, increasing geometrically by a factor of 2.

An example of a radio source where the window centred on the host galaxy, shown as a rectangle, does not contain enough radio information to correctly identify the galaxy as the host. The background image is a 3.6 µm image from SWIRE. The contours show ATLAS radio data and start at 4σ, increasing geometrically by a factor of 2.

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