Correlation of the South Pole 94 data with 100microns and 408 MHz maps
We present a correlation between the ACME/SP94 CMB anisotropy data at 25 to 45 GHz with the IRAS/DIRBE data and the Haslam 408 MHz data. We find a marginal correlation between the dust and the Q-band CMB data but none between the CMB data and the Haslam map. While the amplitude of the correlation wi...
| Main Authors: | , |
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| Format: | Text |
| Language: | unknown |
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arXiv
2001
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| Subjects: | |
| Online Access: | https://dx.doi.org/10.48550/arxiv.astro-ph/0101131 https://arxiv.org/abs/astro-ph/0101131 |
| Summary: | We present a correlation between the ACME/SP94 CMB anisotropy data at 25 to 45 GHz with the IRAS/DIRBE data and the Haslam 408 MHz data. We find a marginal correlation between the dust and the Q-band CMB data but none between the CMB data and the Haslam map. While the amplitude of the correlation with the dust is larger than that expected from naive models of dust emission it does not dominate the sky emission. : 6 pages, 4 figures. Accepted for publication in Astronomy and Astrophysics |
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