Elliptical Beams in CMB Temperature and Polarization Anisotropy Experiments: An Analytic Approach
arXiv:astro-ph/0107346 · doi:10.1103/PhysRevD.65.063003
Abstract
We present an analytic approach to the estimation of beam asymmetry effects in CMB temperature and linear polarization anisotropy experiments. We derive via perturbative expansions simple and accurate results for the case of an elliptical Gaussian window. Our results are applied to investigate the effect of beam ellipticity in the estimation of full-sky polarization correlation functions and the covariance matrix of power spectra. The relevance of this effect is also discussed by forecasting errors including beam asymmetry for current and future CMB experiments.
17 pages, 12 figures. Matches version accepted by PRD: Discussion added on the advantages of introducing a perturbative approach to address beam asymmetry effects, and about the implementation of the results to actual CMB experiments
References in corpus (2)
Cited by in corpus (31)
- The Cosmological Constant and Dark Energy
- Cosmic Microwave Background Anisotropies
- Benchmark Parameters for CMB Polarization Experiments
- The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops
- Planck early results. VI. The High Frequency Instrument data processing
- Xspect, estimation of the angular power spectrum by computing cross-power spectra with analytical error bars
- Peculiar velocity effects in high-resolution microwave background experiments
- Fast Pixel Space Convolution for CMB Surveys with Asymmetric Beams and Complex Scan Strategies: FEBeCoP
- The CMB temperature power spectrum from an improved analysis of the Archeops data
- QuickPol: Fast calculation of effective beam matrices for CMB polarization
- CMB power spectrum estimation using noncircular beams
- Beam deconvolution in noisy CMB maps
- Forecast for the Planck precision on the tensor to scalar ratio and other cosmological parameters
- Full-sky beam convolution for cosmic microwave background applications
- Asymfast, a method for convolving maps with asymmetric main beams
- Data analysis methods for the cosmic microwave background
- PILOT: a balloon-borne experiment to measure the polarized FIR emission of dust grains in the interstellar medium
- Leakage of power from dipole to higher multipoles due to non-symmetric WMAP beam
- CMB power spectrum estimation with non-circular beam and incomplete sky coverage
- Non-Circular beam correction to the CMB power spectrum
- Statistical isotropy violation in WMAP CMB maps resulting from non-circular beams
- Full-sky correlation functions for CMB experiments with asymmetric window functions
- Systematic effects in the measurement of polarization by the PLANCK telescope
- Cosmology Large Angular Scale Surveyor (CLASS): 90 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
- Estimating SI violation in CMB due to non-circular beam and complex scan in minutes
- Ultrafast multireflector physical-optics beam simulations for the HFI instrument on the ESA PLANCK Surveyor
- Effect of noncircularity of experimental beam on CMB parameter estimation
- Dipole leakage and low CMB multipoles
- The CMB Derivatives of Planck's Beam Asymmetry
- Optimal bolometer transfer function deconvolution for CMB experiments through maximum likelihood mapmaking
- Asymmetry and non-random orientation of the inflight effective beam pattern in the WMAP Data