Polarized QPOs from the INTEGRAL polar IGRJ14536-5522 (=Swift J1453.4-5524)
Stephen B. Potter, David A. H. Buckley, Darragh O'Donoghue, Encarni, Romero-Colmenero, James O'Connor, Piet Fourie, Geoff Evans, Craig Sass, Lisa, Crause, Martin Still, O. W. Butters, A.J. Norton, Koji Mukai

TL;DR
This study presents optical spectroscopy, photometry, and polarimetry of the polar IGRJ14536-5522, revealing polarized modulations and first-time detection of 5-6 minute QPOs in circular polarimetry, advancing understanding of accretion processes.
Contribution
First detection of quasi-periodic oscillations in circular polarimetry of a polar, providing new insights into accretion dynamics in magnetic cataclysmic variables.
Findings
Orbital period of 3.1564 hours confirmed.
Circular polarization modulations up to -18%.
Detection of 5-6 minute QPOs in polarimetry.
Abstract
We report optical spectroscopy and high speed photometry and polarimetry of the INTEGRAL source IGRJ14536-5522 (=Swift J1453.4-5524). The photometry, polarimetry and spectroscopy are modulated on an orbital period of 3.1564(1) hours. Orbital circularly polarized modulations are seen from 0 to -18 per cent, unambiguously identifying IGRJ14536-5522 as a polar. Some of the high speed photometric data show modulations that are consistent with quasi-periodic oscillations (QPOs) on the order of 5-6 minutes. Furthermore, for the first time, we detect the (5-6) minute QPOs in the circular polarimetry. We discuss the possible origins of these QPOs. We also include details of HIPPO, a new high-speed photo-polarimeter used for some of our observations.
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