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The rotation measures of 555 extragalactic radio sources are calculated as a result of a large number of new linear polarization measurements carried out at several wavelengths. A summary of references for previous polarization measurements is included, and the procedure for optimizing the number of unambiguous rotation measures is described.
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Simard‐Normandin et al. (Thu,) studied this question.
synapsesocial.com/papers/6a16062250a6b268c6c5b66e — DOI: https://doi.org/10.1086/190709
M. Simard‐Normandin
Nortel (Canada)
P. P. Kronberg
University of Toronto
S. Button
The Astrophysical Journal Supplement Series
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