System equivalent flux density of Stokes I, Q, U, and V of a polarimetric interferometer

Author:

Sutinjo A. T.ORCID,Ung D. C. X.,Sokolowski M.ORCID

Abstract

Aims. We present the system equivalent flux density (SEFD) expressions for all four Stokes parameters: I, Q, U, and V. Methods. The expressions were derived based on our derivation of SEFD I (for Stokes I) and subsequent extensions of that work to phased array and multipole interferometers. The key to the derivation of the SEFD Q, U, and V expressions is to recognize that the noisy estimates of Q, U, and V can be written as the trace of a matrix product. This shows that the SEFD I is a special case, where the general case involves a diagonal or anti-diagonal 2 × 2 matrix interposed in the matrix multiplication. Following this step, the relation between the SEFD for I as well as Q, U, and V immediately becomes evident. Results. We present example calculations for a crossed dipole based on the formulas derived and the comparison between simulation and observation using the Murchison Widefield Array (MWA).

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. PSRDP: A Parallel Processing Method for Pulsar Baseband Data;Research in Astronomy and Astrophysics;2024-01-01

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