Polarization leakage in epoch of reionization windows - I. Low Frequency Array observations of the 3C196 field
Polarization leakage in epoch of reionization windows - I. Low Frequency Array observations of the 3C196 field
复制标题
再电离窗历元的极化泄漏 - I. 3C196 场的低频阵列观测
DOI:
10.1093/mnras/stv1107
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发表时间:
2015
影响因子:
4.8
通讯作者:
Asad K
中科院分区:
文献类型:
--
作者:
Asad K
Detection of the 21-cm signal coming from the epoch of reionization (EoR) is challenging especially because, even after removing the foregrounds, the residual StokesImaps contain leakage from polarized emission that can mimic the signal. Here, we discuss the instrumental polarization of Low Frequency Array (LOFAR) and present realistic simulations of the leakages between Stokes parameters. From the LOFAR observations of polarized emission in the 3C196 field, we have quantified the level of polarization leakage caused by the nominal model beam of LOFAR, and compared it with the EoR signal using power spectrum analysis. We found that at 134–166 MHz, within the central 4° of the field the (Q,U) →Ileakage power is lower than the EoR signal atk< 0.3 Mpc−1. The leakage was found to be localized around a Faraday depth of 0, and the rms of the leakage as a fraction of the rms of the polarized emission was shown to vary between 0.2 and 0.3 per cent, both of which could be utilized in the removal of leakage. Moreover, we could define an ‘EoR window’ in terms of the polarization leakage in the cylindrical power spectrum above the point spread function (PSF)-induced wedge and belowk∥∼ 0.5 Mpc−1, and the window extended up tok∥∼ 1 Mpc−1at allk⊥when 70 per cent of the leakage had been removed. These LOFAR results show that even a modest polarimetric calibration over a field of view of ≲ 4° in the future arrays like Square Kilometre Array will ensure that the polarization leakage remains well below the expected EoR signal at the scales of 0.02–1 Mpc−1.