activity
20242026
most citedInferring the population properties of galactic binaries from LISA's stochastic foreground

1 citations · 1 across the 3 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2026

Population synthesis and detection prospects for Galactic long-period transients with LISA

Arthur G. Suvorov, Nikolaos Karnesis, Valeriya Korol

The recently-discovered long-period radio transients represent a puzzling new class of astrophysical sources, some of which are thought to be compact binary systems emitting a puls…

physics.data-an2026

Learned proposals in trans-dimensional inference are optimal at equilibrium, not during assembly

Argyro Sasli, Nikolaos Karnesis, Minas Karamanis +5

Inferring the dimension of a model - the number of components needed to explain data - jointly with the parameters is a pervasive problem, from counting sources in an image to mixt…

astro-ph.HE20261 cited

Inferring the population properties of galactic binaries from LISA's stochastic foreground

Federico De Santi, Alessandro Santini, Alexandre Toubiana +2

Galactic binaries are expected to be the most numerous LISA sources and to produce a stochastic gravitational-wave foreground whose spectral shape encodes information about the und…

gr-qc2026

Beyond Gaussian Assumptions: A new robust statistical framework for gravitational-wave data analysis

Argyro Sasli, Minas Karamanis, Nikolaos Karnesis +4

Many traditional algorithms applied in gravitational-wave astronomy rely on the assumption of Gaussian noise, a condition not always met. To meet this need, this study extends a ro…

gr-qc2026

Statistics of time and frequency-averaged spectra in gravitational-wave background searches

Quentin Baghi, Nikolaos Karnesis, Jean-Baptiste Bayle

Time series analysis from gravitational-wave detectors often relies on the assumption that time chunks, or frequency bins, are uncorrelated. We discuss the validity of this approxi…

gr-qc2026

Effect of noise characterization on the detection of mHz stochastic gravitational waves

Nikolaos Karnesis, Quentin Baghi, Jean-Baptiste Bayle +1

Pulsar timing arrays' hint for a stochastic gravitational-wave background (SGWB) leverages the expectations of a future detection in the millihertz band, particularly with the LISA…