turbo
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Thank you for that tip, ST. I guess with the contamination of of the time-smearing of pulsar EM arrival times due to magnetic fields, they will not be very good candidates for measuring frequency-dependent effects in the IGM, unless the effect could be shown to be compressed by traveling across lots of IGM (not that we could see get good multi-frequency observations of pulsars in very distant galaxies, anyway).SpaceTiger said:Look up the "dispersion measure".