Velocity distribution of galaxy clustering and their relation to galaxy properties

• Grant number: 16/23563-9
• Support Opportunities: Scholarships in Brazil - Scientific Initiation
• Effective date (Start): January 01, 2017
• Effective date (End): December 31, 2017
• Field of knowledge: Physical Sciences and Mathematics - Astronomy - Extragalactic Astrophysics
• Principal Investigator: Reinaldo Ramos de Carvalho
• Grantee: Lucas Augusto Leardini Siconato
• Host Institution: Instituto Nacional de Pesquisas Espaciais (INPE). Ministério da Ciência, Tecnologia e Inovação (Brasil). São José dos Campos , SP, Brazil
• Associated research grant: 14/11156-4 - What drives the stellar mass growth of Early-Type galaxies? Born or made: the saga continues, AP.TEM

Abstract

We intend to study different methods of analysis of the velocity distribution of galaxies in clusters aiming to establish how Gaussian the distribution is and its reliability. We will be studying the catalog of groups and clusters defined in Yang et al. 2007 (ApJ, 671, 153). The properties of galaxies in these systems are available in the SDSS-DR7. In this project, we will also study the distribution of orbits of galaxies in groups/clusters making use of a program developed by one of the members of the thematic project (MAMPOSSt - Modelling Anisotropy and Mass Profiles of Observed Spherical Systems, Mamon, MNRAS, 429, 3079) thus assessing the relation between Gaussianity and mass profile of the system. (AU)