Table 2

Properties of the ATCA XXL-S observations.

Primary beam FWHM Largest angular scale
Frequency coverage Channels (at 2.1 GHz) Resolution Median noise Area (at 1.809 GHz)
1.076−3.124 GHz 2048 12.3′ 4.76″ 41.3 μJy/beam 23.32 deg2 140″

Notes. The largest angular scale is the largest well-imaged structure the ATCA was sensitive to (at 1.809 GHz, the median effective frequency). The largest source in XXL-S is ~105″ across on the sky.

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