Astrophysical constraints from the SARAS 3 non-detection of the cosmic dawn sky-averaged 21-cm signal

HTJ Bevins, A Fialkov, E de Lera Acedo… - Nature …, 2022 - nature.com
Observations of the redshifted 21-cm line of atomic hydrogen have provided several upper
limits on the 21-cm power spectrum and a tentative detection of the sky-averaged signal at …

Probing the primordial Universe with 21 cm line from cosmic dawn/epoch of reionization

T Minoda, S Saga, T Takahashi… - Publications of the …, 2023 - academic.oup.com
In the most distant reaches of the Universe, the 21 cm hyperfine transition in neutral
hydrogen provides one of the only available tracers of large-scale structure. A number of …

MHD Study of Extreme Space Weather Conditions for Exoplanets With Earth‐Like Magnetospheres: On Habitability Conditions and Radio‐Emission

J Varela, AS Brun, P Zarka, A Strugarek… - Space …, 2022 - Wiley Online Library
The present study aims at characterizing the habitability conditions of exoplanets with an
Earth‐like magnetosphere inside the habitable zone of M and F stars, caused by the direct …

Follow-up radio observations of the Bo\"{o}tis exoplanetary system: Preliminary results from NenuFAR

JD Turner, P Zarka, JM Griessmeier, E Mauduit… - arXiv preprint arXiv …, 2023 - arxiv.org
Studying the magnetic fields of exoplanets will provide valuable information about their
interior structures, atmospheric properties (escape and dynamics), and potential habitability …

MOVES–V. Modelling star–planet magnetic interactions of HD 189733

A Strugarek, R Fares, V Bourrier… - Monthly Notices of …, 2022 - academic.oup.com
Magnetic interactions between stars and close-in planets may lead to a detectable signal on
the stellar disc. HD 189733 is one of the key exosystems thought to harbour magnetic …

Confronting global 21-cm signal with ℤ3 symmetric dark matter models

D Paul, A Dey, AD Banik, S Pal - Journal of Cosmology and …, 2023 - iopscience.iop.org
While the Bbb Z 3 symmetric dark matter models have shown tremendous prospects in
addressing a number of (astro-) particle physics problems, they can leave interesting …

Determining the beaming of Io decametric emissions: a remote diagnostic to probe the Io‐Jupiter interaction

L Lamy, L Colomban, P Zarka, R Prangé… - Journal of …, 2022 - Wiley Online Library
We investigate the beaming of 11 Io‐Jupiter decametric (Io‐DAM) emissions observed by
Juno/Waves, the Nançay Decameter Array, and NenuFAR. Using an up‐to‐date magnetic …

Follow-up of 27 radio-quiet gamma-ray pulsars at 110–190 MHz using the international LOFAR station FR606

JM Grießmeier, DA Smith, G Theureau… - Astronomy & …, 2021 - aanda.org
Context. The Fermi Large Area Telescope has detected over 260 gamma-ray pulsars. About
one quarter of these are labeled as radio-quiet, that is they either have radio flux densities< …

PALANTIR: An updated prediction tool for exoplanetary radio emissions

E Mauduit, JM Grießmeier, P Zarka… - arXiv preprint arXiv …, 2023 - arxiv.org
In the past two decades, it has been convincingly argued that magnetospheric radio
emissions, of cyclotron maser origin, can occur for exoplanetary systems, similarly as solar …

An Active Ribbon Dipole as an Array Element Prototype for the Lunar Very Low Frequency Radio Telescope

PL Tokarsky, AA Konovalenko, JW Modelski - IEEE Access, 2023 - ieeexplore.ieee.org
This work is concerned with a detailed study of an active antenna, which can serve as a
prototype of a phased array antenna element for a future lunar very-low-frequency (VLF) …