output
19942026
most citedThe Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

2.5k citations

Showing 2010 · astro-ph.COShow all

7 papers · 2 filters

astro-ph.CO2010★ 61 cited

The Voronoi Tessellation cluster finder in 2+1 dimensions

Marcelle Soares-Santos, Reinaldo R. de Carvalho, James Annis +6

We present a detailed description of the Voronoi Tessellation (VT) cluster finder algorithm in 2+1 dimensions, which improves on past implementations of this technique. The need fo…

astro-ph.CO2010★ 28 cited

Segregation Effects According to the Evolutionary Stage of Galaxy Groups

Andre L. B. Ribeiro, Paulo A. A. Lopes, Marina Trevisan

We study segregation phenomena in 57 groups selected from the 2PIGG catalog of galaxy groups. The sample corresponds to those systems located in areas of at least 80% redshift cove…

astro-ph.CO2010★ 14 cited

Coupled quintessence with a possible transient accelerating phase

F. E. M. Costa

We discuss some cosmological consequences of a general model of coupled quintessence in which the phenomenological coupling between the cold dark matter and dark energy is a functi…

astro-ph.CO2010★ 49 cited

SPIDER - IV. Optical and NIR color gradients in Early-type galaxies: New Insights into Correlations with Galaxy Properties

F. La Barbera, R. R. de Carvalho, I. G. de la Rosa +3

We present an analysis of stellar population gradients in 4,546 Early-Type Galaxies with photometry in along with optical spectroscopy. A new approach is described which…

astro-ph.CO2010★ 89 cited

Tracing The Sound Horizon Scale With Photometric Redshift Surveys

E. Sanchez, A. Carnero, J. Garcia-Bellido +6

We propose a new method for cosmological parameters extraction using the baryon acoustic oscillation scale as a standard ruler in deep galaxy surveys with photometric determination…

astro-ph.CO2010★ 24 cited

The chemical evolution of IC10

Jun Yin, Laura Magrini, Francesca Matteucci +3

Dwarf irregular galaxies are relatively simple unevolved objects where it is easy to test models of galactic chemical evolution. We attempt to determine the star formation and gas…