Published in

Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 3(445), p. 2198-2213

DOI: 10.1093/mnras/stu1802

Links

Tools

Export citation

Search in Google Scholar

Minor versus major mergers: the stellar mass growth of massive galaxies from z = 3 using number density selection techniques

This paper is available in a repository.
This paper is available in a repository.

Full text: Download

Green circle
Preprint: archiving allowed
Green circle
Postprint: archiving allowed
Green circle
Published version: archiving allowed
Data provided by SHERPA/RoMEO

Abstract

We present a study on the stellar mass growth of the progenitors of local massive galaxies with a variety of number density selections with $n\le1\times10^{-4}\,\rm{Mpc^{-3}}$ (corresponding to $M_*=10^{11.24}\rm{M_{\odot}}$ at z=0.3) in the redshift range $0.3