Astronomy and Astrophysics – Astrophysics – Instrumentation and Methods for Astrophysics
Scientific paper
2010-01-29
Mon. Not. R. Astron. Soc. Volume 408, Issue 2, pages 1029-1050, Oct. 2010
Astronomy and Astrophysics
Astrophysics
Instrumentation and Methods for Astrophysics
18 pages, 13 figures; Replaced to match accepted MNRAS version
Scientific paper
10.1111/j.1365-2966.2010.17174.x
Growing interest in 21 cm tomography has led to the design and construction of broadband radio interferometers with low noise, moderate angular resolution, high spectral resolution, and wide fields of view. With characteristics somewhat different from traditional radio instruments, these interferometers may require new calibration techniques in order to reach their design sensitivities. Self-calibration or redundant calibration techniques that allow an instrument to be calibrated off complicated sky emission structures are ideal. In particular, the large number of redundant baselines possessed by these new instruments makes redundant calibration an especially attractive option. In this paper, we explore the errors and biases in existing redundant calibration schemes through simulations, and show how statistical biases can be eliminated. We also develop a general calibration formalism that includes both redundant baseline methods and basic point source calibration methods as special cases, and show how slight deviations from perfect redundancy and coplanarity can be taken into account.
Liu Adrian
Lutomirski Andrew
Morrison Scott
Tegmark Max
Zaldarriaga Matias
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