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20242026
most citedHydrogen intensity mapping with MeerKAT: Preserving cosmological signal by optimising contaminant separation

12 citations · 22 across the 11 of their papers we have counts for

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astro-ph.CO2026

Emission line stacking on cosmological scales: equivalence to two-point statistics and modelling of the observational effects

Zhaoting Chen, José Luis Bernal

Emission line stacking measurement for cosmological line intensity mapping (LIM) contains not only the average emission line profile of the stacked sources, but usually also the cl…

astro-ph.CO2026

The Super-Sample Covariance of Line-Intensity Mapping Power Spectrum

Sefa Pamuk, José Luis Bernal, Azadeh Moradinezhad Dizgah

In this work, we provide the first derivation of the line-intensity mapping (LIM) power spectrum super-sample covariance (SSC) from first principles, and also derive as a by-produc…

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 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

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…

cs.CV2026

PackForcing: Short Video Training Suffices for Long Video Sampling and Long Context Inference

Xiaofeng Mao, Shaohao Rui, Kaining Ying +4

Autoregressive video diffusion models have demonstrated remarkable progress, yet they remain bottlenecked by intractable linear KV-cache growth, temporal repetition, and compoundin…