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Ewan D. Barr edited considerations.tex
over 8 years ago
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$\log_{10}{\rm DM}= \frac{1}{2.14}(-0.154 + \sqrt{0.0247 + 4.28(13.46+3.86\log_{10}{\nu}+\log_{10}{t_{\rm res}})}$,\\ where the frequency ($\nu$) is defined as the top of the current observing band and the time resolution ($t_{\rm res}$) is defined by SKA1-SYS\_REQ-2961.
\item \textbf{SKA1-SYS\_REQ-XXXX:} \textit{\bf SKA1\_Low Pulsar Timing DM limits.} The SKA1\_Mid when in pulsar timing mode shall time pulsars up to a dispersion measure defined by:\\
$\log_{10}{\rm DM}= \frac{1}{2.14}(-0.154 + \sqrt{0.0247 + 4.28(13.46+3.86\log_{10}{\nu}+\log_{10}{t_{\rm res}})}$,\\
where the frequency ($\nu$) is defined as the centre of the
given coarse frequency channel SKA1\_Low observing band and the time resolution ($t_{\rm res}$) is defined by SKA1-SYS\_REQ-2962.
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