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

S Munshi, FG Mertens, LVE Koopmans… - Astronomy & …, 2024 - aanda.org
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 …

A census of the pulsar population observed with the international LOFAR station FR606 at low frequencies (25–80 MHz)

L Bondonneau, JM Grießmeier, G Theureau… - Astronomy & …, 2020 - aanda.org
Context. To date, only 69 pulsars have been identified with a detected pulsed radio emission
below 100 MHz. A LOFAR-core LBA census and a dedicated campaign with the Nançay …

Constraining the magnetic field geometry of the millisecond pulsar PSR J0030+ 0451 from joint radio, thermal X-ray, and γ-ray emission

J Pétri, S Guillot, L Guillemot, I Cognard… - Astronomy & …, 2023 - aanda.org
Context. With the advent of multi-wavelength electromagnetic observations of neutron stars–
spanning many decades in photon energies–from radio wavelengths up to X-rays and γ …

A LOFAR census of non-recycled pulsars: extending to frequencies below 80 MHz

AV Bilous, L Bondonneau, VI Kondratiev… - Astronomy & …, 2020 - aanda.org
We present the results from the low-frequency (40–78 MHz) extension of the first pulsar
census of non-recycled pulsars carried out with the LOw-Frequency ARray (LOFAR). We …

Dispersion by pulsars, magnetars, fast radio bursts and massive electromagnetism at very low radio frequencies

MJ Bentum, L Bonetti, ADAM Spallicci - Advances in space research, 2017 - Elsevier
Our understanding of the universe relies mostly on electromagnetism. As photons are the
messengers, fundamental physics is concerned in testing their properties. Photon mass …

Sensitivity of an active antenna array element for the low-frequency radio telescope GURT

PL Tokarsky, AA Konovalenko… - IEEE Transactions on …, 2017 - ieeexplore.ieee.org
The recently developed new generation, low-frequency Giant Ukrainian Radio Telescope
(GURT) is built nearby the well-known Ukrainian T-shaped Radio Telescope. The new …

The low-frequency radio telescope NenuFAR

P Zarka, L Denis, M Tagger, J Girard, A Coffre… - URSI GASS …, 2020 - hal.science
NenuFAR is a new, large low-frequency radio telescope, in construction and commissioning
at the Nançay Radioastronomy Observatory, that starts to provide high sensitivity …

Robust distributed calibration of radio interferometers with direction dependent distortions

V Ollier, MN El Korso, A Ferrari, R Boyer, P Larzabal - Signal Processing, 2018 - Elsevier
In radio astronomy, accurate calibration is of crucial importance for the new generation of
radio interferometers. More specifically, because of the potential presence of outliers which …

Barankin bound vs Cramer-Rao bound for interferometric-like array design at low SNR

J Wang, L Bacharach, MN El Korso… - 2023 31st European …, 2023 - ieeexplore.ieee.org
In this paper, we address the antenna array design problem at low signal-to-noise ratio
(SNR). The Cramér-Rao bound (CRB) is the most commonly used criterion to solve the array …

The search for radio emission from exoplanets using LOFAR beam-formed observations: Jupiter as an exoplanet

JD Turner, JM Grießmeier, P Zarka… - Astronomy & …, 2019 - aanda.org
Context. The magnetized solar system planets are strong radio emitters and theoretical
studies suggest that the radio emission from nearby exoplanets in close-in orbits could …