Detection of spin-modulated circular polarisation and radial velocity variations in the long period Intermediate Polar 1RXS J080114.6-462324
We present a comprehensive photometric, spectroscopic, and polarimetric study of the intermediate polar (IP) 1RXS J080114.6-462324, using observations from the South African Astronomical Observatory (SAAO) 1.0-m and 1.9-m telescopes and the Southern African Large Telescope (SALT), complemented by archival TESS photometry. Photometric and photo-polarimetric data reveal a coherent modulation at the white dwarf (WD) spin period. TESS confirms periodicities of 1307.517 s (spin) and 11.803 h (orbital). Photopolarimetric and circular spectropolarimetric measurements show circular polarisation reaching ~+5%, modulated with the WD spin period, consistent with cyclotron emission from an accreting magnetic pole. Time-resolved optical spectra display prominent Balmer (H$\gamma$, H$\beta$, and H$\alpha$) and He\textsc{ii} $\lambda$4686 emission features and additional He\textsc{i} emissions, all exhibiting minimal radial-velocity variations. We detect red-shifted absorption dips adjacent to the He\textsc{ii} and H$\beta$ lines, modulated at the WD spin period; periodogram analysis of the emission lines also yields spin modulation. These observations indicate that the system is a disc-fed, low-inclination IP. The combination of circular polarisation and spin-modulated absorption by infalling accretion curtain material supports this classification. Its comparatively long orbital period among IPs and the detection of polarised emission render 1RXS J080114.6-462324 an appealing candidate for evolutionary studies, potentially offering insight into how magnetic accretion systems evolve toward synchronism at longer orbital periods.