Skip to main content
Article
Investigating Galaxy Clusters In The Infrared
American Institute of Physics (2004)
  • James L. Higdon, Cornell University
  • Sarah J.U. Higdon, Cornell University
  • Terry L. Herter, Cornell University
Abstract
Galaxy clusters preserve important information on the development of large scale structure in the Universe and the formation and evolution of galaxies. It is advantageous to work longward of 1 μm when studying high‐z clusters because of dust obscuration. This is especially true for z>2, where we expect the bulk of star formation to occur in heavily obscured environments. One may also wish to measure emission in the rest‐frame optical and near‐infrared wavelength ranges, which shift to the near and mid‐infrared part of the spectrum for z>1. Two projects are outlined where infrared observations, including those made with the Spitzer Space Telescope, play key roles: an investigation of the mechanism behind the radio Butcher‐Oemler effect in z∼0.5 clusters and a wide field emission line search for clusters of young galaxies at z>2.
Keywords
  • Galaxy Clusters,
  • Infrared telescopes,
  • Space based telescopes,
  • Emission spectra,
  • Galactic evolution
Publication Date
December 10, 2004
DOI
10.1063/1.1848330
Citation Information
James L. Higdon, Sarah J.U. Higdon and Terry L. Herter. "Investigating Galaxy Clusters In The Infrared" American Institute of Physics (2004)
Available at: http://works.bepress.com/sarah_higdon/23/