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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 7.

Measured fluxes (black points) of 11 sources plotted against the published spectra from (PB17; solid line above 50 MHz, dotted line below 50 MHz), (SH12; dashed line), and Baars et al. (1977) (dot-dashed line). Cas A is compared against a spectrum assuming a secular decrease of 0.77% yr–1 (Helmboldt & Kassim 2009).

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