Using cumulative number densities to compare galaxies across cosmic time

Peter S. Behroozi, Danilo Marchesini, Risa H. Wechsler, Adam Muzzin, Casey Papovich, Mauro Stefanon

Research output: Contribution to journalArticlepeer-review

108 Scopus citations

Abstract

Comparing galaxies across redshifts at fixed cumulative number density is a popular way to estimate the evolution of specific galaxy populations. This method ignores scatter in mass accretion histories and galaxy-galaxy mergers, which can lead to errors when comparing galaxies over large redshift ranges (Δz > 1). We use abundance matching in the ΛCDM paradigm to estimate the median change in cumulative number density with redshift and provide a simple fit (+0.16 dex per unit Δz) for progenitors of z = 0 galaxies. We find that galaxy descendants do not evolve in the same way as galaxy progenitors, largely due to scatter in mass accretion histories. We also provide estimates for the 1σ range of cumulative number densities corresponding to galaxy progenitors and descendants. Finally, we discuss some limits on cumulative number density comparisons, which arise due to difficulties measuring physical quantities (e.g., stellar mass) consistently across redshifts. A public tool to calculate cumulative number density evolution for galaxies, as well as approximate halo masses, is available online.

Original languageEnglish (US)
Article numberL10
JournalAstrophysical Journal Letters
Volume777
Issue number1
DOIs
StatePublished - Nov 1 2013
Externally publishedYes

Keywords

  • galaxies: evolution

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'Using cumulative number densities to compare galaxies across cosmic time'. Together they form a unique fingerprint.

Cite this