4.7 Article

A numerical study of 21-cm signal suppression and noise increase in direction-dependent calibration of LOFAR data

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 509, Issue 3, Pages 3693-3702

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stab3233

Keywords

methods: numerical; methods: observational; techniques: interferometric; dark ages; reionization; first stars

Funding

  1. European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme [884760]
  2. Royal Society Dorothy Hodgkin Fellowship
  3. Royal Society Enhancement Award
  4. Science and Technology Facilities Council [ST/I000976/1, ST/T000473/1]
  5. Southeast Physics Network (SEP-Net)
  6. IUCAA, Pune
  7. STFC [ST/T000473/1] Funding Source: UKRI
  8. European Research Council (ERC) [884760] Funding Source: European Research Council (ERC)

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This article investigates the systematic effects in direction-dependent gain calibration in the LOFAR 21-cm EoR experiment. It shows that calibrating short baselines using longer baselines can avoid signal suppression but leads to excess variance. The study demonstrates that regularization algorithms can mitigate this excess variance.
We investigate systematic effects in direction-dependent gain calibration in the context of the Low-Frequency Array (LOFAR) 21-cm Epoch of Reionization (EoR) experiment. The LOFAR EoR Key Science Project aims to detect the 21-cm signal of neutral hydrogen on interferometric baselines of 50-250 lambda. We show that suppression of faint signals can effectively be avoided by calibrating these short baselines using only the longer baselines. However, this approach causes an excess variance on the short baselines due to small gain errors induced by overfitting during calibration. We apply a regularized expectation-maximization algorithm with consensus optimization (sagecal-co) to real data with simulated signals to show that overfitting can be largely mitigated by penalising spectrally non-smooth gain solutions during calibration. This reduces the excess power with about a factor of 4 in the simulations. Our results agree with earlier theoretical analysis of this bias-variance trade off and support the gain-calibration approach to the LOFAR 21-cm signal data.

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