A Morphological Indicator for Comparing Simulated Cosmological Scenarios with Observations

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dc.creatorLega, E.
dc.creatorBijaoui, A.
dc.creatorAlimi, J. -M.
dc.creatorScholl, H.
dc.date1995-10-31
dc.date.accessioned2026-07-07T02:20:21Z
dc.date.available2026-07-07T02:20:21Z
dc.descriptionWe propose a morphological multi-scale analysis of large-scale structures obtained by computer simulations and by observations. Structures are obtained at different scales by applying a wavelet transform on the observed and simulated data. Application of a segmentation algorithm allows a quantitative morphological description of the structures at each scale. The morphological parameter which we propose represents the deviation of a structure from sphericity. The dependence on scale of this simple parameter is shown to characterize in simulations the underlying cosmological model. We compare the HDM, CDM and mixed models with the CfA catalogue. This comparison favours a mixed model containing $65\%$ of CDM, $30\%$ of HDM, and $5\%$ baryonic matter.
dc.descriptionuuencoded compressed postscript file, accepted for publication in Astronomy and Astrophysics
dc.identifierhttps://arxiv.org/abs/astro-ph/9510156
dc.identifierhttp://arxiv.org/abs/astro-ph/9510156
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10187
dc.subjectAstrophysics
dc.titleA Morphological Indicator for Comparing Simulated Cosmological Scenarios with Observations
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