activity
20162025
most citedImproved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR

311 citations · 1.5k across the 29 of their papers we have counts for

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18 papers · 1 filter

astro-ph.CO2025★ 9 cited

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…

astro-ph.CO2024★ 9 cited

Ionospheric contributions to the excess power in high-redshift 21-cm power-spectrum observations with LOFAR

S. A. Brackenhoff, M. Mevius, L. V. E. Koopmans +9

The turbulent ionosphere causes phase shifts to incoming radio waves on a broad range of temporal and spatial scales. When an interferometer is not sufficiently calibrated for the…

astro-ph.CO2024★ 4 cited

The impact of lossy data compression on the power spectrum of the high redshift 21-cm signal with LOFAR

J. K. Chege, L. V. E. Koopmans, A. R. Offringa +8

Current radio interferometers output multi-petabyte-scale volumes of data per year making the storage, transfer, and processing of this data a sizeable challenge. This challenge is…

astro-ph.CO2024★ 15 cited

Beyond the horizon: Quantifying the full sky foreground wedge in the cylindrical power spectrum

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

One of the main obstacles preventing the detection of the redshifted 21-cm signal from neutral hydrogen in the early Universe is the astrophysical foreground emission, which is sev…

astro-ph.CO2024★ 4 cited

Investigating Mutual Coupling in the Hydrogen Epoch of Reionization Array and Mitigating its Effects on the 21-cm Power Spectrum

E. Rath, R. Pascua, A. T. Josaitis +78

Interferometric experiments designed to detect the highly redshifted 21-cm signal from neutral hydrogen are producing increasingly stringent constraints on the 21-cm power spectrum…

astro-ph.CO2023★ 12 cited

Transient RFI environment of LOFAR-LBA at 72-75 MHz: Impact on ultra-widefield AARTFAAC Cosmic Explorer observations of the redshifted 21-cm signal

B. K. Gehlot, L. V. E. Koopmans, S. A. Brackenhoff +13

Measurement of the redshifted 21-cm signal of neutral hydrogen from the Cosmic Dawn (CD) and Epoch of Reionisation (EoR) promises to unveil a wealth of information about the astrop…

astro-ph.CO2023★ 59 cited

First upper limits on the 21 cm signal power spectrum from cosmic dawn from one night of observations with NenuFAR

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

The redshifted 21 cm signal from neutral hydrogen is a direct probe of the physics of the early universe and has been an important science driver of many present and upcoming radio…

astro-ph.CO2023★ 7 cited

Diffuse Sources, Clustering and the Excess Anisotropy of the Radio Synchrotron Background

F. J. Cowie, A. R. Offringa, B. K. Gehlot +4

We present the largest low frequency (120~MHz) arcminute resolution image of the radio synchrotron background (RSB) to date, and its corresponding angular power spectrum of anisotr…

astro-ph.CO2022★ 24 cited

Assessing the impact of two independent direction-dependent calibration algorithms on the LOFAR 21-cm signal power spectrum

H. Gan, F. G. Mertens, L. V. E. Koopmans +11

Detecting the 21-cm signal from the Epoch of Reionisation (EoR) is challenging due to the strong astrophysical foregrounds, ionospheric effects, radio frequency interference and in…

astro-ph.CO2022★ 21 cited

Statistical analysis of the causes of excess variance in the 21 cm signal power spectra obtained with the Low-Frequency Array

H. Gan, L. V. E Koopmans, F. G. Mertens +11

The detection of the 21 cm signal of neutral hydrogen from the Epoch of Reionization (EoR) is challenging due to bright foreground sources, radio frequency interference (RFI), the…

astro-ph.CO2021

Precision Calibration of Radio Interferometers for 21 cm Cosmology with No Redundancy and Little Knowledge of Antenna Beams and the Radio Sky

Aaron Ewall-Wice, Joshua S. Dillon, Bharat Gehlot +3

We introduce CALAMITY, a precision bandpass calibration method for radio interferometry. CALAMITY can solve for direction independent gains with arbitrary frequency structure to th…

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★ 59 cited

Comparing Foreground Removal Techniques for Recovery of the LOFAR-EoR 21cm Power Spectrum

Ian Hothi, Emma Chapman, Jonathan R. Pritchard +10

We compare various foreground removal techniques that are being utilised to remove bright foregrounds in various experiments aiming to detect the redshifted 21cm signal of neutral…

astro-ph.CO2020★ 43 cited

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★ 88 cited

Tight Constraints on the Excess Radio Background at from LOFAR

R. Mondal, A. Fialkov, C. Fling +13

The ARCADE2 and LWA1 experiments have claimed an excess over the Cosmic Microwave Background (CMB) at low radio frequencies. If the cosmological high-redshift contribution to this…

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.CO2020★ 109 cited

Constraining the intergalactic medium at 9.1 using LOFAR Epoch of Reionization observations

R. Ghara, S. K. Giri, G. Mellema +19

We derive constraints on the thermal and ionization states of the intergalactic medium (IGM) at redshift 9.1 using new upper limits on the 21-cm power spectrum measured b…

astro-ph.CO2017★ 290 cited

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 (…