Removal and replacement of interference in tied-array radio pulsar observations using the spectral kurtosis estimator - Archive ouverte HAL Access content directly
Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2022

## Removal and replacement of interference in tied-array radio pulsar observations using the spectral kurtosis estimator

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M. Purver
• Function : Author
C. G. Bassa
• Function : Author
Ismael Cognard
G. H. Janssen
• Function : Author
R. Karuppusamy
• Function : Author
M. Kramer
• Function : Author
K. J. Lee
• Function : Author
J. W. Mckee
• Function : Author
D. Perrodin
• Function : Author
S. Sanidas
• Function : Author
R. Smits
• Function : Author
B. W. Stappers
• Function : Author

#### Abstract

We describe how to implement the spectral kurtosis method of interference removal (zapping) on a digitized signal of averaged power values. Spectral kurtosis is a hypothesis test, analogous to the t-test, with a null hypothesis that the amplitudes from which power is formed belong to a 'good' distribution - typically Gaussian with zero mean - where power values are zapped if the hypothesis is rejected at a specified confidence level. We derive signal-to-noise ratios (SNRs) as a function of amount of zapping for folded radio pulsar observations consisting of a sum of signals from multiple telescopes in independent radio-frequency interference environments, comparing four methods to compensate for lost data with coherent (tied-array) and incoherent summation. For coherently summed amplitudes, scaling amplitudes from non-zapped telescopes achieves a higher SNR than replacing zapped amplitudes with artificial noise. For incoherently summed power values, the highest SNR is given by scaling power from non-zapped telescopes to maintain a constant mean. We use spectral kurtosis to clean a tied-array radio pulsar observation by the Large European Array for Pulsars: the signal from one telescope is zapped with time and frequency resolutions of $6.25\, \mathrm{ms}$ and $0.16\, \mathrm{MHz}$, removing interference, along with 0.27 per cent of 'good' data, giving an uncertainty of $0.25\, \mathrm{\mu \mathrm{ s}}$ in pulse time of arrival (TOA) for PSR J1022+1001. We use a single-telescope observation to demonstrate recovery of the pulse profile shape, with 0.6 per cent of data zapped and a reduction from 1.22 to $0.70\, \mathrm{\mu \mathrm{ s}}$ in TOA uncertainty.

### Dates and versions

insu-03642348 , version 1 (15-04-2022)

### Identifiers

• HAL Id : insu-03642348 , version 1
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• BIBCODE :
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### Cite

M. Purver, C. G. Bassa, Ismael Cognard, G. H. Janssen, R. Karuppusamy, et al.. Removal and replacement of interference in tied-array radio pulsar observations using the spectral kurtosis estimator. Monthly Notices of the Royal Astronomical Society, 2022, 510, pp.1597-1611. ⟨10.1093/mnras/stab3434⟩. ⟨insu-03642348⟩

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