Galaxy mergers at z ≳ 1 in the HUDF: Evidence for a peak in the major merger rate of massive galaxies

R. E. Ryan, S. H. Cohen, Rogier Windhorst, J. Silk

Research output: Contribution to journalArticle

51 Citations (Scopus)

Abstract

We present a measurement of the galaxy merger fraction and number density from observations in the Hubble Ultra Deep Field (HUDF) for 0.5 ≤ z ≤ 2.5. We fit the combination of broadband data and slitless spectroscopy of 1308 galaxies with stellar population synthesis models to select merging systems based on a stellar mass of ≥ 1010 M. When correcting for mass incompleteness, the major merger fraction is not simply proportional to (1 + z)m but appears to peak at zfrac ≃ 1.3 ± 0.4. From this merger fraction, we infer that ∼42% of massive galaxies have undergone a major merger since z ≃ 1. We show that the major merger number density peaks at zdens ≃ 1.2, which marks the epoch where major merging of massive galaxies is most prevalent. This critical redshift is comparable to the peak of the cosmic star formation rate density and occurs roughly 2.6 Gyr earlier in cosmic time than the peak in the number density of the X-ray-selected active galactic nuclei. These observations support an indirect evolutionary link between merging, starburst, and active galaxies.

Original languageEnglish (US)
Pages (from-to)751-757
Number of pages7
JournalAstrophysical Journal
Volume678
Issue number2
DOIs
StatePublished - May 10 2008

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merger
galaxies
broadband data
active galaxies
starburst galaxies
star formation rate
stellar mass
active galactic nuclei
spectroscopy
time measurement
rate
broadband
synthesis
x rays

Keywords

  • Galaxies: evolution
  • Galaxies: formation
  • Galaxies: interactions

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Galaxy mergers at z ≳ 1 in the HUDF : Evidence for a peak in the major merger rate of massive galaxies. / Ryan, R. E.; Cohen, S. H.; Windhorst, Rogier; Silk, J.

In: Astrophysical Journal, Vol. 678, No. 2, 10.05.2008, p. 751-757.

Research output: Contribution to journalArticle

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N2 - We present a measurement of the galaxy merger fraction and number density from observations in the Hubble Ultra Deep Field (HUDF) for 0.5 ≤ z ≤ 2.5. We fit the combination of broadband data and slitless spectroscopy of 1308 galaxies with stellar population synthesis models to select merging systems based on a stellar mass of ≥ 1010 M⊙. When correcting for mass incompleteness, the major merger fraction is not simply proportional to (1 + z)m but appears to peak at zfrac ≃ 1.3 ± 0.4. From this merger fraction, we infer that ∼42% of massive galaxies have undergone a major merger since z ≃ 1. We show that the major merger number density peaks at zdens ≃ 1.2, which marks the epoch where major merging of massive galaxies is most prevalent. This critical redshift is comparable to the peak of the cosmic star formation rate density and occurs roughly 2.6 Gyr earlier in cosmic time than the peak in the number density of the X-ray-selected active galactic nuclei. These observations support an indirect evolutionary link between merging, starburst, and active galaxies.

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