Massive neutrinos leave distinct imprints on specific triangle configurations in the three-point correlation function of halos, with patterns that differ from sigma_8 variations and thus help break their degeneracy.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
representative citing papers
Euclid early release observations of Abell 2390 yield consistent weak lensing mass estimates from three shape catalogs and tomographic bins after contamination corrections.
A vision transformer classifier trained on simulated and real Euclid data recovers all known strong lenses in test sets and finds 8 Grade A plus 26 Grade B new candidates in the Q1 data.
Bulge-disc decomposition on 2445 galaxies with I_E < 21 in Euclid ERO Perseus data shows B/T spanning 0-1, single-Sérsic radii as intermediates, and 0.3 mag median bulge-disc color differences driven by disc-dominated systems.
citing papers explorer
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The imprints of massive neutrinos on the three-point correlation function of large-scale structures
Massive neutrinos leave distinct imprints on specific triangle configurations in the three-point correlation function of halos, with patterns that differ from sigma_8 variations and thus help break their degeneracy.
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Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390
Euclid early release observations of Abell 2390 yield consistent weak lensing mass estimates from three shape catalogs and tomographic bins after contamination corrections.
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Euclid Quick Data Release (Q1). AstroVink: A vision transformer approach to find strong gravitational lens systems
A vision transformer classifier trained on simulated and real Euclid data recovers all known strong lenses in test sets and finds 8 Grade A plus 26 Grade B new candidates in the Q1 data.
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Euclid: Galaxy morphology and photometry from bulge-disc decomposition of Early Release Observations
Bulge-disc decomposition on 2445 galaxies with I_E < 21 in Euclid ERO Perseus data shows B/T spanning 0-1, single-Sérsic radii as intermediates, and 0.3 mag median bulge-disc color differences driven by disc-dominated systems.