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Table · dataset · 2025

Matter power spectrum reconstruction

Listed in IVOA Registry (Virtual Observatory)

Direct measurements of the matter power spectrum, Pm (k, z), provide a powerful tool to investigate observed tensions between models of structure growth while also testing the internal consistency of cosmological probes.

Description

We analyse cosmic shear data from the final data release of the Kilo- Degree Survey (KiDS), presenting a deprojected Pm (k, z), measured in up to three redshift bins. Compared to analyses using previous KiDS releases, we find improved internal consistency in the z<~0.7 regime.

At large scales, k<~0.1h/Mp, our power spectrum reconstruction aligns with {LAMBDA}CDM predictions with a density fluctuation amplitude {sigma}_8_=0.81. Furthermore, at small scales, k=3-20h/Mpc, the average matter power spectrum is suppressed by 30%+/-10% (stat.)+/-4% (sys.) with 2.8{sigma} significance relative to a dark-matter-only model, consistent with expectations of strong baryonic feedback.

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Catalogue records · 2

Topics

Inferred from text
Astronomical sciences 73%
Provenance · 1 source records, 8 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/703/l313 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].anzsrc:group:5101enrichment · IVOA Registrytaxonomy-embedding@1.1.0title+keywords+description (73%)
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0