| Issue |
A&A
Volume 368, Number 3, March IV 2001
|
|
|---|---|---|
| Page(s) | 760 - 765 | |
| Section | Astrophysical processes | |
| DOI | https://doi.org/10.1051/0004-6361:20010061 | |
| Published online | 15 March 2001 | |
Correlation of the South Pole 94 data with 
m and 408 MHz maps
1
Physique Corpusculaire et Cosmologie, CNRS-IN2P3, Collège de France, 11 place M. Berthelot, 75231 Paris Cedex, France
2
Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA
Corresponding author: J.-Ch. Hamilton, hamilton@cdf.in2p3.fr
Received:
11
October
2000
Accepted:
8
January
2000
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.
Key words: cosmic microwave background / cosmology: observations
© ESO, 2001
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.