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Extreme Starlight Polarization Efficiency toward ζ Ophiuchi: A Case for Line-of-sight Foreground Subtraction

  • Authors: Jordan A. Bartlett, Henry A. Kobulnicky

Jordan A. Bartlett and Henry A. Kobulnicky 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 4.

RGB image of the foreground-corrected target field, formatted as in Figure 1. The ζ Oph Group and Far Group have been corrected by the average values of the ζ Oph Group (﹩\bar{q}=-0.76 \% ﹩ and ﹩\bar{u}=-1.22 \% ﹩). Because they are nearer than the foreground, polarizing dust, the Near Group targets have not been corrected.

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