K. Wiersema, P. A. Curran, T. Kruehler, A. Melandri, E. Rol, R. L. C. Starling, N. R. Tanvir, A. J. van der Horst, S. Covino, J. P. U. Fynbo, P. Goldoni, J. Gorosabel, J. Hjorth, S. Klose, C. G. Mundell, P. T. O'Brien, E. Palazzi, R. A. M. J. Wijers, V. D'Elia, P. A. Evans, R. Filgas, A. Gomboc, J. Greiner, C. Guidorzi, L. Kaper, S. Kobayashi, C. Kouveliotou, A. J. Levan, A. Rossi, A. Rowlinson, I. A. Steele, A. de Ugarte Postigo, S. D. Vergani
[Abridged] A number of phenomena have been observed in GRB afterglows that defy explanation by simple versions of the standard fireball model, leading to a variety of new models. Polarimetry can be a major independent diagnostic of afterglow physics, probing the magnetic field properties and internal structure of the GRB jets. In this paper we present the first high quality multi-night polarimetric light curve of a Swift GRB afterglow, aimed at providing a well calibrated dataset of a typical afterglow to serve as a benchmark system for modelling afterglow polarisation behaviour. In particular, our dataset of the afterglow of GRB 091018 (at redshift z=0.971) comprises optical linear polarimetry (R band, 0.13 - 2.3 days after burst); circular polarimetry (R band) and near-infrared linear polarimetry (Ks band). We add to that high quality optical and near-infrared broadband light curves and spectral energy distributions as well as afterglow spectroscopy. The linear polarisation varies between 0 and 3%, with both long and short time scale variability visible. We find an achromatic break in the afterglow light curve, which corresponds to features in the polarimetric curve. We find that the data can be reproduced by jet break models only if an additional polarised component of unknown nature is present in the polarimetric curve. We probe the ordered magnetic field component in the afterglow through our deep circular polarimetry, finding P_circ < 0.15% (2 sigma), the deepest limit yet for a GRB afterglow, suggesting ordered fields are weak, if at all present. Our simultaneous R and Ks band polarimetry shows that dust induced polarisation in the host galaxy is likely negligible.
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http://arxiv.org/abs/1203.4265
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