A fundamental figure of merit for radio polarimeters
arXiv:0908.2330 · doi:10.1109/TAP.2011.2123862
Abstract
This paper has been withdrawn to allow publication elsewhere.
This paper has been withdrawn
References in corpus (4)
- Radio Astronomical Polarimetry and Point-Source Calibration
- Deep Westerbork observations of Abell 2256 at 350 MHz
- A generalised Measurement Equation and van Cittert-Zernike theorem for wide-field radio astronomical interferometry
- Correcting the Polarization Leakage Phases and Amplitudes Throughout the Primary Beam of an Interferometer
Cited by in corpus (9)
- An ultra-wide bandwidth (704 to 4032 MHz) receiver for the Parkes radio telescope
- The MeerKAT Telescope as a Pulsar Facility: System verification and early science results from MeerTime
- A Fast Radio Burst with frequency-dependent polarization detected during Breakthrough Listen observations
- SKA Aperture Array Verification System: Electromagnetic modeling and beam pattern measurements using a micro UAV
- Polarization leakage in epoch of reionization windows: II. Primary beam model and direction dependent calibration
- MWA Tied-Array Processing II: Polarimetric Verification and Analysis of two Bright Southern Pulsars
- Intrinsic Instrumental Polarization and High-Precision Pulsar Timing
- Low-cost, Low-loss, Ultra-wideband Compact Feed for Interferometric Radio Telescopes
- Quantification of propagation modes in an astronomical instrument from its radiation pattern