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The CHILES Continuum and Polarization Survey. I. Survey Design and Noise Characterization

  • Authors: Nicholas M. Luber, Min S. Yun, Hansung B. Gim, Daniel Krista-Kelsey, D.J. Pisano, Emmanuel Momjian, Chris Hales

Nicholas M. Luber et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 1.

The CHILES Con Pol field, defined as the 20% (blue circle) and 50% (orange circle) of the VLA primary beam at 1.4 GHz, overlaid on the COSMOS HST coverage (A. M. Koekemoer et al. 2007). In addition, to provide context for the extensive multiwavelength coverage in the COSMOS field, we present the footprints of just a few of the many surveys the JWST COSMOS-Web field-of-view is presented in red (C. M. Casey et al. 2023), the AxTEC submillimeter survey is presented in magenta (I. Aretxaga et al. 2011), the CFHT NUV survey is presented in black (P. Capak et al. 2007), and the GAMA G10 region of reprocessed COSMOS photometry and spectroscopic is shown in green (S. K. Andrews et al. 2017).

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