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Prospects for multiwavelength polarization observations of GRB afterglows and the case GRB 030329

S. Klose·E. Palazzi·N. Masetti·B. Stecklum·J. Greiner·D. H. Hartmann·H. M. Schmid
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Abstract

We explore the prospects for simultaneous, broad-band, multiwavelength polarimetric observations of GRB afterglows. We focus on the role of cosmic dust in GRB host galaxies on the observed percentage polarization of afterglows in the optical/near-infrared bands as a function of redshift. Our driving point is the afterglow of GRB 030329, for which we obtained polarimetric data in the R band and K band simultaneously about 1.5 days after the burst. We argue that polarimetric observations can be very sensitive to dust in a GRB host, because dust can render the polarization of an afterglow wavelength-dependent. We discuss the consequences for the interpretation of observational data and emphasize the important role of very early polarimetric follow-up observations in all bands, when afterglows are still bright, to study the physical properties of dust and magnetic fields in high-z galaxies.

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S. Klose, E. Palazzi, N. Masetti, B. Stecklum, J. Greiner, D. H. Hartmann, H. M. Schmid. 2004-03-21. Prospects for multiwavelength polarization observations of GRB afterglows and the case GRB 030329. https://doi.org/10.1051/0004-6361%3A20041024

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