dc.contributor.author | Symeonidis, M. | |
dc.contributor.author | Rigopoulou, D. | |
dc.contributor.author | Huang, J. S. | |
dc.contributor.author | Davis, M. | |
dc.contributor.author | Ashby, M. L. N. | |
dc.contributor.author | Barmby, P. | |
dc.contributor.author | Egami, E. | |
dc.contributor.author | Fazio, G. G. | |
dc.contributor.author | Le Floc'h, E. | |
dc.contributor.author | Rieke, G. H. | |
dc.contributor.author | Willner, S. P. | |
dc.contributor.author | Wilson, Graham Wallace | |
dc.date.accessioned | 2015-05-11T19:29:43Z | |
dc.date.available | 2015-05-11T19:29:43Z | |
dc.date.issued | 2007-05-01 | |
dc.identifier.citation | Symeonidis, M. et al. (2007). "AEGIS: Infrared Spectral Energy Distributions of MIPS 70 μm-selected Sources." Astrophysical Journal Letters, 660(1):L73-L76. http://www.dx.doi.org/10.1086/517928. | en_US |
dc.identifier.uri | http://hdl.handle.net/1808/17707 | |
dc.description | This is the publisher's version, also available electronically from http://iopscience.iop.org/1538-4357/660/1/L73/. | en_US |
dc.description.abstract | We present 0.5-160 μm spectral energy distributions (SEDs) of galaxies, detected at 70 μm with the Multiband Imaging Photometer for Spitzer (MIPS), using broadband imaging data from Spitzer and ground-based telescopes. Spectroscopic redshifts, in the range 0.2 ≤ z ≤ 1.5, have been measured as part of the Deep Extragalactic Evolutionary Probe 2 (DEEP2) project. On the basis of the SEDs, we explore the nature and physical properties of the sources. Using the optical spectra, we derive Hβ and [O II]-based star formation rates (SFRs) that are 10-100 times lower than SFR estimates based on IR and radio. The median offset in SFR between optical and IR is reduced by a factor of ~3 when we apply a typical extinction correction. We investigate mid- to far-infrared correlations for low-redshift (>0.5) and high-redshift (0.5 < z < 1.2) bins. Using this unique "far-infrared"-selected sample, we derive an empirical mid- to far-infrared relationship that can be used to estimate the infrared energy budget of galaxies in the high-redshift universe. Our sample can be used as a template to translate far-infrared luminosities into bolometric luminosities for high-redshift objects. | en_US |
dc.publisher | American Astronomical Society | en_US |
dc.subject | Galaxies: fundamental parameters | en_US |
dc.subject | Galaxies: high-redshift | en_US |
dc.subject | Infrared: galaxies | en_US |
dc.title | AEGIS: Infrared Spectral Energy Distributions of MIPS 70 μm-selected Sources | en_US |
dc.type | Article | |
kusw.kuauthor | Wilson, Graham Wallace | |
kusw.kudepartment | Physics and Astronomy | en_US |
dc.identifier.doi | 10.1086/517928 | |
kusw.oaversion | Scholarly/refereed, publisher version | |
kusw.oapolicy | This item does not meet KU Open Access policy criteria. | |
dc.rights.accessrights | openAccess | |