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20112026
most citedPlanck 2015 results. XVII. Constraints on primordial non-Gaussianity

507 citations · 4.8k across the 27 of their papers we have counts for

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astro-ph.IM2026

Scalable Bayesian data curation for next-generation radio experiments

S. A. K. Leeney, E. de Lera Acedo, W. J. Handley +42

Next-generation radio telescopes produce data volumes that preclude manual quality assessment, yet data curation remains essential for science. We present a general, fully automati…

astro-ph.IM2026

Optimisation of calibration sources for global 21-cm experiments: the REACH case

Adarsh Kumar Dash, Dominic Anstey, Harry T. J. Bevins +41

The spin-flip 21-cm signal from the Cosmic Dawn and the Epoch of Reionization is an essential probe of the conditions that led to the formation of the first luminous objects in the…

astro-ph.IM2026

Circuit Modeling for In Situ 21 cm Radiometer Calibration

Gary Vincent Charles Allen, Saurabh Pegwal, Dirk de Villiers +42

Recent experiments in cosmology, particularly those aimed at detecting the faint, redshifted, global 21 cm hydrogen line (depth < ~200 mK, z > 7.5), have imposed stringent new requ…

astro-ph.IM2015★ 74 cited

Planck 2015 results. VII. HFI TOI and beam processing

Planck Collaboration, R. Adam, P. A. R. Ade +225

The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polari…

astro-ph.IM2015★ 62 cited

Planck 2015 results. II. Low Frequency Instrument data processing

Planck Collaboration, P. A. R. Ade, N. Aghanim +213

We present an updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline, associated with the 2015 data release. We point out the places where our re…

astro-ph.IM2011★ 190 cited

Planck early results: first assessment of the High Frequency Instrument in-flight performance

Planck HFI Core Team, P. A. R. Ade, N. Aghanim +163

The Planck High Frequency Instrument (HFI) is designed to measure the temperature and polarization anisotropies of the Cosmic Microwave Background and galactic foregrounds in six w…