Modeling the evolution of infrared galaxies: clustering of galaxies in the cosmic infrared background

@article{Penin2012ModelingTE,
  title={Modeling the evolution of infrared galaxies: clustering of galaxies in the cosmic infrared background},
  author={Aur'elie P'enin and Olivier Dor'e and Guilaine Lagache and Matthieu B'ethermin},
  journal={Astronomy and Astrophysics},
  year={2012},
  volume={537}
}
Context. Star-forming galaxies are highly biased tracers of the underlying dark matter density field. Their clustering can be studied through the cosmic infrared background (CIB) anisotropies. These anisotropies have been measured from 100 μm to 2 mm in the past few years. Aims. In this paper, we present a fully parametric model allowing joint analysis of these recent observations. Methods. To develop a coherent model at various wavelengths, we rely on two building blocks. The first one… 
The redshift evolution of the distribution of star formation among dark matter halos as seen in the infrared
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Context. The measurement of the anisotropies in the cosmic infrared background (CIB) is a powerful means of studying the evolution of galaxies and large-scale structures. These anisotropies have been
Constraining thermal dust emission in distant galaxies with number counts and angular power spectra
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Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation
The multi-frequency capability of the Planck satellite provides information both on the integrated history of star formation (via the cosmic infrared background, or CIB) and on the distribution of
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