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20052026
most citedImproved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR

311 citations · 1.4k across the 22 of their papers we have counts for

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6 papers · 1 filter

astro-ph.CO2021★ 30 cited

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

M. Mevius, F. Mertens, L. V. E. Koopmans +14

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…

astro-ph.CO2020

The AARTFAAC Cosmic Explorer: observations of the 21-cm power spectrum in the EDGES absorption trough

B. K. Gehlot, F. G. Mertens, L. V. E. Koopmans +12

The 21-cm absorption feature reported by the EDGES collaboration is several times stronger than that predicted by traditional astrophysical models. If genuine, a deeper absorption…

astro-ph.CO2020★ 311 cited

Improved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR

F. G. Mertens, M. Mevius, L. V. E Koopmans +23

A new upper limit on the 21-cm signal power spectrum at a redshift of is presented, based on 141 hours of data obtained with the Low-Frequency Array (LOFAR). The an…

astro-ph.CO2017

Upper limits on the 21-cm Epoch of Reionization power spectrum from one night with LOFAR

A. H. Patil, S. Yatawatta, L. V. E. Koopmans +25

We present the first limits on the Epoch of Reionization (EoR) 21-cm HI power spectra, in the redshift range , using the Low-Frequency Array (LOFAR) High-Band Antenna (…

astro-ph.CO2012★ 130 cited

The Scale of the Problem : Recovering Images of Reionization with GMCA

Emma Chapman, Filipe B. Abdalla, J. Bobin +8

The accurate and precise removal of 21-cm foregrounds from Epoch of Reionization redshifted 21-cm emission data is essential if we are to gain insight into an unexplored cosmologic…

astro-ph.CO2009★ 106 cited

Non-parametric foreground subtraction for 21cm epoch of reionization experiments

Geraint Harker, Saleem Zaroubi, Gianni Bernardi +12

An obstacle to the detection of redshifted 21cm emission from the epoch of reionization (EoR) is the presence of foregrounds which exceed the cosmological signal in intensity by or…