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
Page 9 and 10: Pulsar ObservationsObservational fr
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Page 15 and 16: Pulsar Surveysa “position” on t
Page 17 and 18: Green Bank Ultimate PulsarProcessin
Page 19 and 20: Pulsar Timing ArraysNew Feed & Rx S
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Pulsar Timing Arrays Current and Future Instrumentation - DCC

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