Assembly of the red sequence in infrared-selected galaxy clusters from the irac shallow cluster survey

Gregory F. Snyder, Mark Brodwin, Conor M. Mancone, Gregory R. Zeimann, S. A. Stanford, Anthonyh Gonzalez, Daniel Stern, Peter R M Eisenhardt, Michael J I Brown, Arjun Dey, Buell Tomasson Jannuzi, Saul Perlmutter

Research output: Contribution to journalArticle

45 Citations (Scopus)

Abstract

We present results for the assembly and star formation histories (SFHs) of massive (∼L*) red sequence galaxies (RSGs) in 11 spectroscopically confirmed, infrared-selected galaxy clusters at 1.0 < z < 1.5, the precursors to present-day massive clusters with M ∼1015 M . Using rest-frame optical photometry, we investigate evolution in the color and scatter of the RSG population, comparing with models of possible SFHs. In contrast to studies of central cluster galaxies at lower redshift (z < 1), these data are clearly inconsistent with the continued evolution of stars formed and assembled primarily at a single, much earlier time. Specifically, we find that the colors of massive cluster galaxies at z ≈1.5 imply that the bulk of star formation occurred at z ∼3, whereas by z ≈1 their colors imply formation at z ∼2; therefore these galaxies exhibit approximately the same luminosity-weighted stellar age at 1 < z < 1.5. This likely reflects star formation that occurs over an extended period, the effects of significant progenitor bias, or both. Our results generally indicate that massive cluster galaxy populations began forming a significant mass of stars at z ≳ 4, contained some red spheroids by z ≈1.5, and were actively assembling much of their final mass during 1 < z < 2 in the form of younger stars. Qualitatively, the slopes of the cluster color-magnitude relations are consistent with no significant evolution relative to local clusters.

Original languageEnglish (US)
Article number114
JournalAstrophysical Journal
Volume756
Issue number2
DOIs
StatePublished - Sep 10 2012
Externally publishedYes

Fingerprint

assembly
galaxies
star formation
color
stars
history
histories
stellar luminosity
spheroids
assembling
photometry
slopes

Keywords

  • galaxies
  • galaxies: clusters: general
  • galaxies: elliptical and lenticular, cD
  • galaxies: evolution
  • galaxies: formation
  • photometry

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Snyder, G. F., Brodwin, M., Mancone, C. M., Zeimann, G. R., Stanford, S. A., Gonzalez, A., ... Perlmutter, S. (2012). Assembly of the red sequence in infrared-selected galaxy clusters from the irac shallow cluster survey. Astrophysical Journal, 756(2), [114]. https://doi.org/10.1088/0004-637X/756/2/114

Assembly of the red sequence in infrared-selected galaxy clusters from the irac shallow cluster survey. / Snyder, Gregory F.; Brodwin, Mark; Mancone, Conor M.; Zeimann, Gregory R.; Stanford, S. A.; Gonzalez, Anthonyh; Stern, Daniel; Eisenhardt, Peter R M; Brown, Michael J I; Dey, Arjun; Jannuzi, Buell Tomasson; Perlmutter, Saul.

In: Astrophysical Journal, Vol. 756, No. 2, 114, 10.09.2012.

Research output: Contribution to journalArticle

Snyder, GF, Brodwin, M, Mancone, CM, Zeimann, GR, Stanford, SA, Gonzalez, A, Stern, D, Eisenhardt, PRM, Brown, MJI, Dey, A, Jannuzi, BT & Perlmutter, S 2012, 'Assembly of the red sequence in infrared-selected galaxy clusters from the irac shallow cluster survey', Astrophysical Journal, vol. 756, no. 2, 114. https://doi.org/10.1088/0004-637X/756/2/114
Snyder, Gregory F. ; Brodwin, Mark ; Mancone, Conor M. ; Zeimann, Gregory R. ; Stanford, S. A. ; Gonzalez, Anthonyh ; Stern, Daniel ; Eisenhardt, Peter R M ; Brown, Michael J I ; Dey, Arjun ; Jannuzi, Buell Tomasson ; Perlmutter, Saul. / Assembly of the red sequence in infrared-selected galaxy clusters from the irac shallow cluster survey. In: Astrophysical Journal. 2012 ; Vol. 756, No. 2.
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