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19962026
most citedDecision Tree Classifiers for Star/Galaxy Separation

94 citations · 587 across the 27 of their papers we have counts for

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18 papers · 1 filter

astro-ph2008★ 47 cited

The Northern Sky Optical Cluster Survey III: A Cluster Catalog Covering Pi Steradians

R. R. Gal, P. A. A. Lopes, R. R. de Carvalho +3

We present the complete galaxy cluster catalog from the Northern Sky Optical Cluster Survey, a new, objectively defined catalog of candidate galaxy clusters at z<0.25 drawn from th…

astro-ph2008★ 2 cited

Enlightening the structure and dynamics of Abell 1942

H. V. Capelato, D. Proust, G. B. LIma Neto +2

We present a dynamical analysis of the galaxy cluster Abell 1942 based on a set of 128 velocities obtained at the European Southern Observatory. Data on individual galaxies are pre…

astro-ph2006★ 36 cited

X-ray Galaxy Clusters in NoSOCS: Substructure and the Correlation of Optical and X-ray Properties

P. A. A. Lopes, R. R. de Carvalho, H. V. Capelato +5

We present a comparison of optical and X-ray properties of galaxy clusters in the northern sky. We determine the recovery rate of X-ray detected clusters in the optical as a functi…

astro-ph2004★ 13 cited

Merging of Low-Mass Systems and the Origin of the Fundamental Plane

E. A. Evstigneeva, R. R. de Carvalho, A. L. Ribeiro +1

We present a new set of dissipationless N-body simulations to examine the feasibility of creating bright ellipticals (following the Kormendy relation) by hierarchically merging pre…

astro-ph2003★ 1 cited

The cluster of galaxies Abell 376

D. Proust, H. V. Capelato, G. Hickel +3

We present a dynamical analysis of the galaxy cluster Abell 376 based on a set of 73 velocities, most of them measured at Pic du Midi and Haute-Provence observatories and completed…

astro-ph2002★ 37 cited

"Fundamental-Plane"-Like Relations From Collisionless Stellar Dynamics: A Comparison of Mergers and Collapses

Christine C. Dantas, Hugo V. Capelato, Andre L. B. Ribeiro +1

We present a new set of dissipationless N-body simulations aiming to better understand the pure dynamical aspects of the ``Fundamental Plane'' (FP) of elliptical galaxies. We have…