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An Ultradeep Multiband VLA Survey of the Faint Radio Sky (COSMOS-XS): Source Catalog and Number Counts

  • Authors: D. van der Vlugt, H. S. B. Algera, J. A. Hodge, M. Novak, J. F. Radcliffe, D. A. Riechers, H. Röttgering, V. Smolčić, and F. Walter

2021 The Astrophysical Journal 907 5.

  • Provider: AAS Journals

Caption: Figure 13.

Fitted angular size, θ (geometric mean), as a function of integrated flux density at 3 GHz. Unresolved sources fall below the red dotted line giving the minimum size of a source. The minimum size was derived using the envelope from Section 3.2. The blue shaded region shows the maximum size a source of a given integrated flux density can have before dropping below the peak brightness detection threshold, where the range reflects the range of rms noise in the 3 GHz image.

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