Dust Attenuation in High Redshift Galaxies -- 'Diamonds in the Sky'

@article{Scoville2014DustAI,
  title={Dust Attenuation in High Redshift Galaxies -- 'Diamonds in the Sky'},
  author={Nicholas Scoville and Andreas L. Faisst and Peter Capak and Yuko Kakazu and Gongjie Li and Charles L. Steinhardt},
  journal={arXiv: Astrophysics of Galaxies},
  year={2014}
}
We use observed optical to near infrared spectral energy distributions (SEDs) of 266 galaxies in the COSMOS survey to derive the wavelength dependence of the dust attenuation at high redshift. All of the galaxies have spectroscopic redshifts in the range z = 2 to 6.5. The presence of the CIV absorption feature, indicating that the rest-frame UV-optical SED is dominated by OB stars, is used to select objects for which the intrinsic, unattenuated spectrum has a well-established shape. Comparison… Expand

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