most citedImproved upper limits on the 21-cm signal power spectrum at and from an optimal field observed with NenuFAR

11 citations · 20 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.CO202511 cited

Improved upper limits on the 21-cm signal power spectrum at and from an optimal field observed with NenuFAR

S. Munshi, F. G. Mertens, J. K. Chege +19

We report the deepest upper limits to date on the power spectrum of the 21-cm signal during the Cosmic Dawn (redshifts: ), using four nights of observations with NenuFAR. The…

astro-ph.CO2025

Mitigating incoherent excess variance in high-redshift 21 cm observations with multi-output cross-Gaussian process regression

S. Munshi, L. V. E. Koopmans, F. G. Mertens +8

Systematic effects that limit the achievable sensitivity of current low-frequency radio telescopes to the 21 cm signal are among the foremost challenges in observational 21 cm cosm…

astro-ph.CO2025

First upper limits on the 21-cm signal power spectrum of neutral hydrogen at from the LOFAR 3C196 field

E. Ceccotti, A. R. Offringa, F. G. Mertens +16

The redshifted 21-cm signal of neutral hydrogen from the Epoch of Reionization (EoR) can potentially be detected using low-frequency radio instruments such as the Low-Frequency Arr…

astro-ph.IM20259 cited

Near-field imaging of local interference in radio interferometric data: Impact on the redshifted 21 cm power spectrum

S. Munshi, F. G. Mertens, L. V. E. Koopmans +24

Radio-frequency interference (RFI) is a major systematic limitation in radio astronomy, particularly for science cases requiring high sensitivity, such as 21 cm cosmology. Traditio…

astro-ph.IM2025

Robust direction-dependent gain-calibration of beam-modelling errors far from the target field

S. A. Brackenhoff, A. R. Offringa, M. Mevius +8

Many astronomical questions require deep, wide-field observations at low radio frequencies. Phased arrays like LOFAR and SKA-low are designed for this, but have inherently unstable…

astro-ph.CO2025

Spectral modelling of Cygnus A between 110 and 250 MHz. Impact on the LOFAR 21-cm signal power spectrum

E. Ceccotti, A. R. Offringa, L. V. E. Koopmans +15

Studying the redshifted 21-cm signal from the the neutral hydrogen during the Epoch of Reionization and Cosmic Dawn is fundamental for understanding the physics of the early univer…