Figure 8 from The Radio Sky at Meter Wavelengths: m-mode Analysis Imaging with the OVRO-LWA

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The Radio Sky at Meter Wavelengths: m-mode Analysis Imaging with the OVRO-LWA

Authors: Michael W. Eastwood, Marin M. Anderson, Ryan M. Monroe, Gregg Hallinan, Benjamin R. Barsdell, Stephen A. Bourke, M. A. Clark, Steven W. Ellingson, Jayce Dowell, Hugh Garsden, Lincoln J. Greenhill, Jacob M. Hartman, Jonathon Kocz, T. Joseph W. Lazio, Danny C. Price, Frank K. Schinzel, Gregory B. Taylor, Harish K. Vedantham, Yuankun Wang, and David P. Woody

2018 The Astronomical Journal 156 32.

Provider: AAS Journals

Caption: Figure 8.

These eight panels illustrate (with a Mollweide projection and logarithmic color scale) the eight full-sky maps generated with Tikhonov-regularized m-mode analysis imaging and the OVRO-LWA. Each map covers the sky north of δ = −30° with angular resolution of ∼15′. Eight bright sources have been removed from each map (Cyg A, Cas A, Vir A, Tau A, Her A, Hya A, 3C 123, and 3C 353). The small blank region near l = +45.°7, b = −47.°9 corresponds to the location of the Sun during the observation period. A detailed summary of the properties of each map is given in Table 1.

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