The Galactic dust as a foreground to Cosmic Microwave Background maps

@article{Dupac2004TheGD,
  title={The Galactic dust as a foreground to Cosmic Microwave Background maps},
  author={Xavier Dupac and J-Ph. Bernard and Nathalie Boudet and Martin Giard and J-M. Lamarre and C. M'eny and François Pajot and Isabelle Ristorcelli},
  journal={arXiv: Astrophysics},
  year={2004},
  pages={89-92}
}
We present results obtained with the PRONAOS balloon-borne experiment on interstellar dust. In particular, the submillimeter / millimeter spectral index is found to vary between roughly 1 and 2.5 on small scales (3.5′ resolution). This could have implications for component separation in Cosmic Microwave Background maps. 

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