| Issue |
A&A
Volume 534, October 2011
|
|
|---|---|---|
| Article Number | L8 | |
| Number of page(s) | 5 | |
| Section | Letters | |
| DOI | https://doi.org/10.1051/0004-6361/201117846 | |
| Published online | 14 October 2011 | |
Online material
Temperature excess in the M 31 regions for the non foreground-reduced WMAP maps.
 |
Fig. 4
In the W, V, and Q bands, the 1σ (green lines), 2σ (brown lines), and 3σ (red lines) excess temperature contrast (in mk/pixel) curves, along with the mean profile (pink line close) for 500 random control fields. The observed temperature contrast profile in the M 31 disk (with 1σ errors) is given in red. The non foreground-reduced WMAP maps are used here. |
| Open with DEXTER | |
 |
Fig. 5
As above (in the W, V, and Q bands) the 1σ (green lines), 2σ (brown lines), and 3σ (red lines) excess temperature contrast (in mk/pixel) curves along with the mean profile (pink line close) for 500 random control fields. The real temperature contrast profile in the M 31 halo up to 20° (with 1σ errors) is given in red. |
| Open with DEXTER | |
© ESO, 2011
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