Detection of the 21-cm signal coming from the epoch of reionization (EoR) is challenging especially because, even after removing the foregrounds, the residual Stokes I maps 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) → I leakage power is lower than the EoR signal...
Aims: This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to...
Aims. This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to...
Aims: This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to...
Detection of the 21-cm signal coming from the epoch of reionization (EoR) is challenging especially ...
Detection of the 21-cm signal coming from the epoch of reionization (EoR) is challenging especially ...
Leakage of diffuse polarized emission into Stokes I caused by the polarized primary beam of the inst...
The farther we look in space, the earlier we see in time. By observing a radio signal of 21cm wavele...
Leakage of diffuse polarized emission into Stokes I caused by the polarized primary beam of the inst...
Leakage of polarized Galactic diffuse emission into total intensity can potentially mimic the 21-cm ...
The farther we look in space, the earlier we see in time. By observing a radio signal of 21cm wavele...
Jelic V, de Bruyn AG, Mevius M, et al. Initial LOFAR observations of epoch of reionization windows I...
Aims: This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to...
Aims. This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to...
Aims: This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to...
Detection of the 21-cm signal coming from the epoch of reionization (EoR) is challenging especially ...
Detection of the 21-cm signal coming from the epoch of reionization (EoR) is challenging especially ...
Leakage of diffuse polarized emission into Stokes I caused by the polarized primary beam of the inst...
The farther we look in space, the earlier we see in time. By observing a radio signal of 21cm wavele...
Leakage of diffuse polarized emission into Stokes I caused by the polarized primary beam of the inst...
Leakage of polarized Galactic diffuse emission into total intensity can potentially mimic the 21-cm ...
The farther we look in space, the earlier we see in time. By observing a radio signal of 21cm wavele...
Jelic V, de Bruyn AG, Mevius M, et al. Initial LOFAR observations of epoch of reionization windows I...
Aims: This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to...
Aims. This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to...
Aims: This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to...