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Author

L. Moscardini

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Review Open access Sep 2026

Observation-driven simulations of strong-lensing galaxy clusters

Galaxy clusters are the most powerful strong lenses; they greatly magnify the flux of distant and faint sources. Strong lensing also allows for the reconstruction of their mass distribution with sim1% accuracy and enables the investigation of cosmological parameters. The number of known systems of this type is bound to...

L. Leuzzi, M. Meneghetti, A. Adam et al. · 0 citations
Review Open access Sep 2026

Euclid preparation. CXIII. Simulated galaxy catalogues for non-standard cosmological models

Stage-IV galaxy surveys will provide the opportunity to test cosmological models and the underlying theory of gravity with unparalleled precision. In this context, it is crucial for the Euclid mission to leverage its spectroscopic and photometric probes to systematically investigate and incorporate non-standard cosmolo...

M.-A. Breton, P. Fosalba, S. Ávila et al. · 0 citations
Review Sep 2026

Euclid. A two-point correlation approach to diagnosing star-related systematics in the Euclid spectroscopic survey

The Euclid spectroscopic survey will measure galaxy clustering with unprecedented precision, requiring stringent control of observational and instrumental systematics. Star-related effects may contaminate spectroscopic images through photometric persistence and imperfect masking of stars. We characterized their impact...

Euclid Collaboration I. Risso, B. Granett, E. Branchini et al. · 0 citations

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