Abstract
We discuss how deep Keck observations (spectroscopy+polarimetry) can be used to constrain and separate the different components contributing to the rest-frame UV-optical continuum of 3C radio galaxies at z ∼1. We also show preliminary results of modeling of their Spectral Energy Distributions (SEDs).
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Cimatti, A., Di Alighieri, S.S. (1998). “Dissecting” 3C Radio Galaxies At Redshift ∼1. In: Bremer, M.N., Jackson, N., Pérez-Fournon, I. (eds) Observational Cosmology. Astrophysics and Space Science Library, vol 226. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5238-9_5
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DOI: https://doi.org/10.1007/978-94-011-5238-9_5
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