Fig. 4 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. 4.

Encircled flux as a function of angular radius. The source is Mars. A map is generated with a rectangular grid of spacing 18^{﹩\arcsec﹩} (1 pixel). The encircled flux is determined by adding the signal values for pixels interior to a given radius. In computing the fraction of total flux, we have extrapolated that 10% of the total flux lies beyond the edges of the map.

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