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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 4.

Difference in the effective polarization spectrum from dust calculated by the power-law fitting for the dust optical depth. The line styles of the curves correspond to the frequency bands used for fitting. The thin dotted curve is the residual when the dust temperature is misestimated as Td = 17 K. The gray colored regions correspond to r < 3 × 10−4, 3 × 10−3, and 0.01 in order of darkness.

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