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Date and Time of the Query: 2019-06-20 T14:17:09 PDT
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For refcode 2008ApJ...688..122H:
Retrieve 16 NED objects in this reference.
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2008ApJ...688..122H Near- and Mid-Infrared Photometry of High-Redshift 3CR Sources Haas, Martin; Willner, S. P.; Heymann, Frank; Ashby, M. L. N.; Fazio, G. G.; Wilkes, Belinda J.; Chini, Rolf; Siebenmorgen, Ralf Abstract. Using the Spitzer Space Telescope, we have obtained 3.6-24 micron photometry of 38 radio galaxies and 24 quasars from the 3CR (Third Cambridge Revised Catalog of Radio Sources) at redshift 1<z<2.5. This 178 MHz selected sample is unbiased with respect to orientation and therefore suited to study orientation-dependent effects in the most powerful active galactic nuclei (AGNs). Quasar and radio galaxy subsamples matched in isotropic radio luminosity are compared. The quasars all have similar spectral energy distributions (SEDs), nearly constant in {nu}F_{nu}_ through the rest 1.6-10 micron range, consistent with a centrally heated dust distribution that outshines the host galaxy contribution. The radio galaxy SEDs show larger dispersion, but the mean radio galaxy SED declines from rest 1.6 to 3 micron and then rises from 3 to 8 micron. The radio galaxies are on average a factor 3-10 less luminous in this spectral range than the quasars. These characteristics are consistent with composite emission from a heavily reddened AGN plus starlight from the host galaxy. The mid-infrared colors and radio to mid-infrared spectral slopes of individual galaxies are also consistent with this picture. Individual galaxies show different amounts of extinction and host galaxy starlight, consistent with the orientation-dependent unified scheme. Key words: Galaxies: Active, Infrared: Galaxies, Galaxies: Quasars: General
Retrieve 16 NED objects in this reference.
Please click here for ADS abstract

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