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20012014
most citedShapley Supercluster Survey (ShaSS): Galaxy Evolution from Filaments to Cluster Cores

43 citations · 131 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2014★ 43 cited

Shapley Supercluster Survey (ShaSS): Galaxy Evolution from Filaments to Cluster Cores

P. Merluzzi, G. Busarello, C. P. Haines +11

We present an overview of a multi-wavelength survey of the Shapley supercluster (SSC; z~0.05) covering a contiguous area of 260 h^-2_70 Mpc^2 including the supercluster core. The p…

astro-ph.CO2009★ 3 cited

Sersic galaxy with Sersic halo models of early-type galaxies: a tool for N-body simulations

G. Coppola, F. La Barbera, M. Capaccioli

We present spherical, non-rotating, isotropic models of early-type galaxies with stellar and dark-matter components both described by deprojected Sersic density profiles, and prove…

astro-ph2008★ 17 cited

Gauging the dark matter fraction in a S0 galaxy at z=0.47 through gravitational lensing from deep HST/ACS imaging

G. Covone, M. Paolillo, N. R. Napolitano +9

We analyze a new gravitational lens, OAC-GL J1223-1239, serendipitously found in a deep I-band image of the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS). The lens…

astro-ph2008★ 9 cited

CMB Anisotropy Induced by a Moving Straight Cosmic String

O. S. Sazhina, M. V. Sazhin, V. N. Sementsov +4

We showed that the part of strings could be detected by optical method is only 20% from the total available amount of such objects, therefore the gravitational lensing method has t…

astro-ph2006

The Environmental Dependencies of Star-formation and the Origin of the Bimodality in Galaxy Properties

C. P. Haines, A. Gargiulo, A. Mercurio +4

We examine the origins of the bimodality observed in the global properties of galaxies by comparing the environmental dependencies of star-formation for giant and dwarf galaxy popu…

astro-ph2002★ 5 cited

Age, Metallicity and Star Formation History of Cluster Galaxies at z~0.3 F

P. Merluzzi, F. La Barbera, M. Massarotti +2

We investigate the color-magnitude distribution in the rich cluster AC 118 at z=0.31. The sample is selected by the photometric redshift technique, allowing to study a wide range o…