Abstract
We investigate the anisotropy in cosmic microwave background Planck maps due to the coupling between its beam asymmetry and uneven scanning strategy. Introducing a pixel space estimator based on the temperature gradients, we find a highly significant (~20σ) preference for these to point along ecliptic latitudes. We examine the scale dependence, morphology and foreground sensitivity of this anisotropy, as well as the capability of detailed Planck simulations to reproduce the effect, which is crucial for its removal, as we demonstrate in a search for the weak-lensing signature of cosmic defects.
Original language | English |
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Pages (from-to) | 750-754 |
Number of pages | 5 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 443 |
Issue number | 1 |
DOIs | |
State | Published - 1 Jan 2014 |
Externally published | Yes |
Keywords
- Cosmic background radiation
- Cosmology: observations
- Cosmology: theory
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science