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CMB Shadows: The Effect of Interstellar Extinction on Cosmic Microwave Background Polarization and Temperature Anisotropy

  • Authors: Masashi Nashimoto, Makoto Hattori, and Yuji Chinone

2020 The Astrophysical Journal Letters 895 L21.

  • Provider: AAS Journals

Caption: Figure 3.

Difference in the effective polarization emission from dust estimated by the single-power-law fitting for the effective polarization emission. The line styles of the curves correspond to the frequency bands used for fitting. The gray colored regions correspond to r < 3 × 10−4, 3 × 10−3, and 0.01 in order of darkness.

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