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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 2.

The rms map of the 10 GHz observation before primary beam correction. The image size is ﹩41\,{\mathrm{arcmin}}^{2}﹩. The rms map is created with PyBDSF. The red circle indicates the HPBW of the primary beam at 10 GHz, which corresponds to ﹩4\buildrel{\,\prime}\over{.} 5﹩. The gray scale shows the rms noise from 0.8σ to 1.2σ, where σ = 0.41 μJy beam−1 The contours are plotted at [0.38, 0.39, 0.41] μJy beam−1.

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