Pulsar Timing Arrays Current and Future Instrumentation - DCC

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$Numerical simulation of diffraction grating alignment and ... - DCC$

<strong>Timing</strong> Precision• Assume σ TOA ≤ 100 nsMay be necessary, but not sufficientconditionWSNRPσ TOA, n=WSNR• W pulse width• SNR signal-to-noise ratio• Assumes sufficient calibration oftelescope systemOther contributions can include pulse-phasejitter, uncorrected propagation effects
Radio Telescope
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Page 7 and 8: Radio TelescopeTNoise Temperature
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Pulsar Timing Arrays Current and Future Instrumentation - DCC

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