An iterative destriping technique for diffuse background polarization data
arXiv:astro-ph/0302276 · doi:10.1051/0004-6361:20030200
Abstract
We describe a simple but effective iterative procedure specifically designed to destripe Q and U Stokes parameter data as those collected by the SPOrt experiment onboard the International Space Station (ISS). The method is general enough to be useful for other experiments, both in polarization and total intensity. The only requirement for the algorithm to work properly is that the receiver knee frequency must be lower than the signal modulation frequency, corresponding in our case to the ISS orbit period. Detailed performances of the technique are presented in the context of the SPOrt experiment, both in terms of added rms noise and residual correlated noise.
Accepted for publication by A&A (8 pages, 6 figures)
References in corpus (13)
- Statistics of Cosmic Microwave Background Polarization
- 9286 Stars: An Agglomeration of Stellar Polarization Catalogs
- Microwave Background Constraints on Cosmological Parameters
- Foregrounds and Forecasts for the Cosmic Microwave Background
- Measuring Polarization In Cosmic Microwave Background
- How to make maps from CMB data without losing information
- CMB mapping experiments: a designer's guide
- Detectability of Inflationary Gravitational Waves with Microwave Background Polarization
- The Planck-LFI instrument: analysis of the 1/f noise and implications for the scanning strategy
- Destriping of Polarized Data in a CMB Mission with a Circular Scanning Strategy
- The power-law behaviours of angular spectra of polarized Galactic synchrotron
- Limits Due to Instrumental Polarisation in CMB Experiments at Microwave Wavelengths
- Polarized Microwave Emission from Dust
Cited by in corpus (14)
- Fast estimation of polarization power spectra using correlation functions
- Destriping CMB temperature and polarization maps
- The Sky Polarization Observatory
- Measuring Planck beams with planets
- Antenna Instrumental Polarization and its Effects on E- and B-Modes for CMBP Observations
- The Parkes Galactic Meridian Survey (PGMS): observations and CMB polarization foreground analysis
- A polarized synchrotron template for CMBP experiments after WMAP data
- A New approach for a Galactic Synchrotron Polarized Emission Template in the Microwave Range
- Polarized Diffuse Emission at 2.3 GHz in a High Galactic Latitude Area
- Growing Supermassive Black Holes by Chaotic Accretion
- On the wavelet analysis of CMB time ordered data: application to Archeops
- The synchrotron foreground and CMB temperature-polarization cross correlation power spectrum from the first year WMAP data
- Making Maps from Planck LFI 30GHz Data with Asymmetric Beams and Cooler Noise
- Effects of Thermal Fluctuations in the SPOrt Experiment