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263 documents correspondants.

Prépublication · 2026 arXiv EN

Unifying spherical convolutions through lifting

We develop a unified description of convolution on the sphere by lifting to the rotation group. A number of definitions of spherical convolution have been proposed, differing in whether the kernel is axisymmetric or directional, whether the output is on the sp...

J. D. McEwen #math-ph
Prépublication · 2026 arXiv EN

The Redshift-Space Galaxy Power Spectrum at Two-Loop Order

Contemporary large-scale structure analyses center around the galaxy power spectrum, modeled with one-loop perturbation theory. This description naturally breaks down at large wavenumbers, prohibiting the extraction of cosmological information from small-scale...

Oliver H. E. Philcox #astro-ph.CO
Prépublication · 2026 arXiv EN

The origin of the large heavy element contents of warm Jupiters

Planet interior models have revealed that warm Jupiters should harbor large heavy element masses (up to 30-40% of the planetary mass). Within the pebble drift and evaporation scenario, inward drifting pebbles can evaporate and enrich the inner disc with vapor...

Bertram Bitsch #astro-ph.EP
Prépublication · 2026 arXiv EN

Assessing PLATO's Discovery Potential across Different Observing Strategies

The PLATO mission, planned to launch in spring 2027, will observe a fixed Southern field, LOPS2, for at least 2 years with the goal of discovering and deriving precise parameters for planets as small as Earth around FGK dwarfs and sub-giants. Afterwards, PLATO...

Yoshi Nike Emilia Eschen, Michelle Kunimoto et al. #astro-ph.EP
Prépublication · 2026 arXiv EN

Detecting redshift space distortions with forthcoming 21cm intensity maps from MeerKLASS

Redshift space distortions (RSD) provide a powerful measurement of structure formation in modern cosmology. In this work, we explore the potential of 21cm intensity mapping with the MeerKAT Large Area Synoptic Survey (MeerKLASS) to detect RSD and probe gravity...

Daniel Tassie, Steven Cunnington et al. #astro-ph.CO
Prépublication · 2026 arXiv EN

Star Cluster Ecology VIII. -- Dynamically Forming S-Type and $α$Centauri-like Systems

Aims: To analyse the impact of dynamically formed binaries emerging naturally from various star cluster environments on already established planetary systems. Methods: Numerical simulations replicating the star-forming region NGC 1333 are conducted. We conside...

Erwan Hochart, Simon Portegies Zwart #astro-ph.EP