A Panoramic Mid-infrared Survey of Two Distant Clusters
| dc.creator | Geach, J. E. | |
| dc.creator | Smail, Ian | |
| dc.creator | Ellis, R. S. | |
| dc.creator | Moran, S. M. | |
| dc.creator | Smith, G. P. | |
| dc.creator | Treu, T. | |
| dc.creator | Kneib, J. -P. | |
| dc.creator | Edge, A. C. | |
| dc.creator | Kodama, T. | |
| dc.date | 2006-06-06 | |
| dc.date.accessioned | 2026-07-07T10:39:12Z | |
| dc.date.available | 2026-07-07T10:39:12Z | |
| dc.description | (abridged) We present panoramic Spitzer MIPS 24um observations covering 9x9Mpc (25'x25') fields around two massive clusters, Cl0024+16 and MS0451-03, at z=0.39 and z=0.55. Our observations cover a very wide range of environments within these clusters, from high-density regions around the cores out to the turn-around radius. Cross-correlating the mid-infrared catalogs with deep optical and near-infrared imaging of these fields, we investigate the optical/near-infrared colors of the mid-infrared sources. We find excesses of mid-infrared sources with optical/near-infrared colors expected of cluster members in the two clusters and test this selection using spectroscopically confirmed 24um members. The much more significant excess is associated with Cl0024+16, whereas MS0451-03 has comparatively few mid-infrared sources. The mid-infrared galaxy population in Cl0024+16 appears to be associated with dusty star-forming galaxies (typically redder than the general cluster population by up to A_V~1-2 mags) rather than emission from dusty tori around active galactic nuclei (AGN) in early-type hosts. The inferred total-infrared star-formation rates in Cl0024+16 are typically >5x greater than those found from a similar Halpha survey, indicating significant obscured activity in the cluster population. We find evidence for strong evolution of the level of dust-obscured star-formation in dense environments out to z=0.5, analogous to the rise in fraction of optically-selected star-forming galaxies seen in clusters and the field out to similar redshifts. However, there are clearly significant cluster-to-cluster variations in the populations of mid-infrared sources, probably reflecting differences in the intracluster media and recent dynamical evolution of these systems. | |
| dc.description | 13 pages, 6 figures, accepted for publication in ApJ | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0606110 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0606110 | |
| dc.identifier | Astrophys.J.649:661-672,2006 | |
| dc.identifier | doi:10.1086/506469 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/180946 | |
| dc.subject | Astrophysics | |
| dc.title | A Panoramic Mid-infrared Survey of Two Distant Clusters | |
| dc.type | text |