Infrared Spectral Energy Distributions of Z ∼ 0.7 Star-forming Galaxies

@inproceedings{XZ2007InfraredSE,
  title={Infrared Spectral Energy Distributions of Z ∼ 0.7 Star-forming Galaxies},
  author={Z XZ and D H.A.WennerM. and B EF},
  year={2007}
}
We analyze the infrared (IR) spectral energy distributions (SEDs) for 10µm < λ rest < 100µm for ∼ 600 galaxies at z ∼ 0.7 in the extended Chandra Deep Field South by stacking their Spitzer 24, 70 and 160 µm images. We place interesting constraints on the average IR SED shape in two bins: the brightest 25% of z ∼ 0.7 galaxies detected at 24 µm, and the remaining 75% of individually-detected galaxies. Galaxies without individual detections at 24 µm were not well-detected at 70 µm and 160 µm even… CONTINUE READING
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