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20002025
most citedThe Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations

273 citations · 2k across the 65 of their papers we have counts for

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Showing 2011Show all

8 papers · 1 filter

astro-ph.CO2011★ 1 cited

Development of the Red Sequence in Galaxy Clusters

Noelia Jiménez, Sofía A. Cora, Analía Smith Castelli +1

We investigate the origin of the color-magnitude relation (CMR) observed in cluster galaxies by using a combination of a cosmological N-body simulation of a cluster of galaxies and…

astro-ph.CO2011★ 34 cited

The bright end of the colour-magnitude relation of cluster galaxies

Noelia Jiménez, Sofía A. Cora, Lilia P. Bassino +2

We investigate the development of the red sequence (RS) of cluster galaxies by using a semi-analytic model of galaxy formation. Results show good agreement between the general tren…

astro-ph.GA2011

Chemical effects on the development of the colour-magnitude relation of cluster galaxies

Noelia Jiménez, Sofía A. Cora, Lilia P. Bassino +2

We investigate the development of the colour-magnitude re- lation (CMR) of cluster galaxies. This study is carried out using a semi- analytic model of galaxy formation and evolutio…

astro-ph.CO2011

Modeling the Color Magnitude Relation for Galaxy Clusters

Noelia Jimenez, Sofia A. Cora, Analia Smith Castelli +1

We investigate the origin of the colour-magnitude relation (CMR) observed in cluster galaxies by using a combination of a cosmological N-body simulation of a cluster of galaxies an…

astro-ph.GA2011

The Color-Magnitude Relation of Cluster Galaxies: Observations and Model Predictions

Noelia Jimenez, Analia Smith Castelli, Sofia A. Cora +1

We investigate the origin of the color-magnitude relation (CMR) observed in cluster galaxies by using a combination of cosmological N-body/SPH simulations of galaxy clusters, and a…

astro-ph.CO2011★ 10 cited

Ram pressure profiles in galaxy groups and clusters

Tomás E. Tecce, Sofía A. Cora, Patricia B. Tissera

Using a hybrid method which combines non-radiative hydrodynamical simulations with a semi-analytic model of galaxy formation, we determine the ram pressure as a function of halocen…