activity
20232026
most citedHydrogen intensity mapping with MeerKAT: Preserving cosmological signal by optimising contaminant separation

12 citations · 24 across the 26 of their papers we have counts for

collaborators

28 papers

astro-ph.CO2026

Cosmological Inference with Gravitational-Wave Dark Sirens and 21-cm Intensity Mapping: Forecasts for LIGO-Virgo-KAGRA with MeerKAT and SKAO

Dounia Nanadoumgar-Lacroze, Konstantin Leyde, Steven Cunnington +8

Gravitational waves (GWs) and 21-cm intensity mapping (IM) are emerging as complementary cosmological probes: GWs provide direct luminosity-distance measurements, while neutral-hyd…

astro-ph.CO2026

JESSNet: Joint dEconvolution and Sparse Separation Network for HI 21 cm foreground cleaning

Athanasia Gkogkou, Victor Bonjean, Jean-Luc Starck +3

Foreground cleaning is a major challenge for H\,{\sc i} 21 cm intensity mapping, particularly in the presence of a chromatic instrumental beam that couples angular foreground struc…

astro-ph.CO2026

Cosmology beyond standard sirens: cross-correlation of gravitational waves and neutral hydrogen intensity mapping

Matteo Schulz, Ulyana Dupletsa, Andrea Cozzumbo +8

We explore the potential of cross-correlation between gravitational wave (GW) events and neutral hydrogen (HI) intensity mapping surveys to serve as an independent cosmological pro…

astro-ph.CO2026

Modeling the HI-Halo Connection: Evolution, Scatter, and a Halo-based Prescription for 21-cm Mock Catalogs

Mohd Kamran, Gabriella De Lucia, Marta Spinelli +3

The redshifted 21-cm line of neutral hydrogen (HI) is a powerful tracer of large-scale structure, and post-reionization HI intensity mapping is emerging as a competitive cosmologic…

astro-ph.CO2026

Overview: Cosmology with the SKAO

Marta Spinelli, Ian Harrison, Richard A. Battye +5

The SKA telescopes will revolutionise our ability to do cosmology at radio wavelengths, via both their own data and in synergy with other wavelengths. SKAO will be the first instru…

astro-ph.IM2026

Advancing Astrophysics with the SKA II

Anna Bonaldi, Tyler L. Bourke, Philippa Hartley +45

Advancing Astrophysics with the SKA II (AASKAII), written by our science community, outlines the transformative scientific advances that will be enabled by the SKA telescopes. In t…

astro-ph.CO2026

Cosmology with HI Intensity Mapping

Laura Wolz, Gabriele Autieri, José Luis Bernal +18

The redshifted spectral emission from neutral hydrogen (HI) at rest wavelength 21 cm can be used as a tracer of large-scale structure and its evolution. Within the HI intensity map…

astro-ph.CO2026

meer21cm: an Analysis Pipeline and Comprehensive Toolkit for HI Intensity Mapping

Zhaoting Chen, Steven Cunnington, Daniel Tassie +23

We present meer21cm, a comprehensive python package for cosmological data analysis of single-dish HI intensity mapping surveys. This package is simple to use, with a modularised co…

astro-ph.CO2026

Cosmology from HI galaxy surveys with the SKA

Ainulnabilah Nasirudin, Philip Bull, Ziad Sakr +8

The 21cm line from neutral hydrogen is expected to be a ubiquitous (albeit faint) tracer of galaxies in the late Universe. With SKAO-MID, large wide-field surveys of several millio…

astro-ph.CO2026

Cosmology with Multi-Wavelength Line Intensity Mapping Synergies in the SKAO Era

Debanjan Sarkar, Suman Majumdar, Chandra Shekhar Murmu +21

Line intensity mapping (LIM) has emerged as a powerful tool for surveying the large-scale structure of the Universe across cosmic time by measuring spatial fluctuations in the cumu…

astro-ph.CO2026

Cosmology with Intensity Mapping via Statistics Beyond the Power Spectrum in the SKAO Era

Suman Majumdar, Debanjan Sarkar, Leon Noble +38

The cosmological distribution of neutral hydrogen (HI) during the post-reionization era is highly non-Gaussian due to the underlying non-linear structure formation, complex galaxy…

astro-ph.CO2026

Methodological Frontiers in 21-cm Intensity Mapping: the Treatment of Systematics and Foreground Contamination

Marta Spinelli, Matilde Barberi-Squarotti, José Luis Bernal +29

The distribution of neutral hydrogen (HI) in the post-reionization universe traces the cosmic large-scale structure and therefore serves as a powerful cosmological probe. An effici…

astro-ph.CO2026

Cosmology from Synergies Between SKAO Surveys and Gravitational Wave Observations

Tessa Baker, Alberto Colombo, Steven Cunnington +11

Both radio surveys and gravitational wave observations have the potential to probe unprecedented volumes in the Universe with systematics independent of existing cosmological probe…

astro-ph.CO2026

Cosmology with Tully-Fisher HI Galaxy Surveys

Joël Mayor, Anthony Carr, Khaled Said +7

The SKA Observatory will enable measurements of the Tully-Fisher relation for statistical samples of HI selected galaxies out to unprecedented depths and redshifts thanks to its un…

astro-ph.CO2026

HI Simulations for Cosmology with the SKA Observatory

Tommaso Ronconi, Gabriella De Lucia, Marta Spinelli +15

We present a comparative overview of state-of-the-art methods for modelling the distribution of neutral hydrogen (HI) in the post-reionization Universe, developed in preparation fo…

astro-ph.CO2026

Single-dish HI Intensity Mapping with the SKAO: Precursor Progress with MeerKAT's Large Area Synoptic Survey (MeerKLASS)

Steven Cunnington, Jingying Wang, Mario G. Santos +16

Using the SKAO to map the intensity of neutral hydrogen's 21cm emission line will be a golden opportunity to constrain models of cosmology. To access the largest cosmological scale…

astro-ph.CO2026

Radio sirens: inferring with binary black holes and neutral hydrogen in the era of the Einstein Telescope and the SKA Observatory

Ulyana Dupletsa, Simone Mastrogiovanni, Marta Spinelli +11

A new synergy between gravitational waves (GWs) and the study of the large-scale structure of the Universe is now emerging. Along this line of research, we combine simulated observ…

astro-ph.CO2026

Beyond power spectrum to unveil systematics on HI intensity maps

Pauline Gorbatchev, Jean-Luc Starck, Stefano Camera +1

HI intensity mapping is a promising technique to probe large-scale structure, traditionally analyzed via two-point statistics such as the angular power spectrum. This technique has…

astro-ph.CO2025★ 1 cited

Foreground removal in HI 21 cm intensity mapping under frequency-dependent beam distortions

Athanasia Gkogkou, Victor Bonjean, Jean-Luc Starck +2

Neutral hydrogen (HI) intensity mapping with single-dish experiments is a powerful approach for probing cosmology in the post-reionization epoch. However, the presence of bright fo…

astro-ph.CO2025

Revealing cosmological fluctuations in 21cm intensity maps with MeerKLASS: from maps to power spectra

Steven Cunnington, Matilde Barberi-Squarotti, José Luis Bernal +8

Mapping the integrated 21cm emission line from dark matter-tracing neutral hydrogen gas is the primary science goal for MeerKLASS (MeerKAT's Large Area Synoptic Survey). Prior to t…

astro-ph.IM2025★ 1 cited

A Decentralized Framework for Radio-interferometric Image Reconstruction

S. Wang, S. Mignot, S. Prunet +3

The advent of large aperture arrays, such as the ones currently under construction for the SKA project, allows for observing the Universe in the radio-spectrum at unprecedented res…

astro-ph.CO2025

Weighing neutrinos with 21cm Intensity Mapping at the SKAO

Gabriele Autieri, Maria Berti, Marta Spinelli +2

We explore the constraining power of future 21cm intensity mapping (IM) observations at the SKAO, focusing primarily on the sum of neutrino masses, . We forecast observations…

astro-ph.IM2025

Karabo: A versatile SKA Observation Simulation Framework

Rohit Sharma, Simon Felix, Luis Fernando Machado Poletti Valle +12

Karabo is a versatile Python-based software framework simplifying research with radio astronomy data. It bundles existing software packages into a coherent whole to improve the eas…

astro-ph.CO2025★ 9 cited

Emission-line Stacking of 21cm Intensity Maps with MeerKLASS: Inference Pipeline and Application to the L-band Deep-field Data

Zhaoting Chen, Steven Cunnington, Alkistis Pourtsidou +11

We present a novel analysis of observational systematics through the emission-line stacking of the MeerKLASS L-band deep-field intensity maps, following the detection in arXiv:2407…