Fig. 3 from Submillimeter Array Polarimetry with Hertz

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Submillimeter Array Polarimetry with Hertz

Authors: C. Darren Dowell, Roger H. Hildebrand, David A. Schleuning, John E. Vaillancourt, Jessie L. Dotson, Giles Novak, Tom Renbarger, and Martin Houde

Dowell et al. 1998 The Astrophysical Journal 504 588.

Provider: AAS Journals

Caption: Fig. 3.

Intensity as a function of angular radius. The source, Mars, had an angular diameter of 12﹩\farcs﹩5 at the time of the observations. Each point corresponds to an average of measurements from several pixels. In the center of the map, the grid spacing was 9^{﹩\arcsec﹩}. At the edge of the map, the grid spacing was 18^{﹩\arcsec﹩}. The intensity has been normalized to 1.0 at the peak. The FWHM of the profile is 24^{﹩\arcsec﹩}.

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