Rapidly-Responding Optical Polarimetry of GRB afterglows with Hiroshima 1.5-m Telescope and One-shot Wide-field Polarimeter

Astronomy and Astrophysics – Astronomy

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Polarimetry, Gamma-Ray Sources (Astronomical), Astronomical Observatories, Polarimetry, Gamma-Ray Sources, Gamma-Ray Bursts, Observatories And Site Testing

Scientific paper

We have developed an optical wide-field polarimeter, HOWPol, which employs a wedged double Wollaston prism and enables us to derive linear polarization (i.e., Stokes Q/I and U/I) from only a single exposure. We successfully performed observation for the afterglow of GRB 091208B. Its first exposure started ~150 seconds after the gamma-ray trigger. Our preliminary result suggests that the early afterglow was significantly polarized, larger than a few percent.

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