Abstract
The Global Magneto-Ionic Medium Survey (GMIMS) is a project to map the diffuse polarized emission over the entire sky, Northern and Southern hemispheres, from 300 MHz to 1.8 GHz. With an angular resolution of 30-60 arcmin and a frequency resolution of 1 MHz or better, GMIMS will provide the first spectro-polarimetric data set of the large-scale polarized emission over the entire sky, observed with single-dish telescopes. GMIMS will provide an invaluable resource for studies of the magneto-ionic medium of the Galaxy in the local disk, halo, and its transition.
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Wolleben, M., Landecker, T. L., Carretti, E., Dickey, J. M., Fletcher, A., Gaensler, B. M., … Taylor, A. R. (2008). GMIMS: The Global Magneto-Ionic Medium Survey. In Proceedings of the International Astronomical Union (Vol. 4, pp. 89–90). Cambridge University Press. https://doi.org/10.1017/S1743921309030117
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