The radio spectral energy distribution of infrared-faint radio sources

The radio spectral energy distribution of infrared-faint radio sources

<strong>Context.</strong>Infrared-faint radio sources (IFRS) are a class of radio-loud (RL) active galactic nuclei (AGN) at high redshifts (z ≥ 1.7) that are characterised by their relative infrared faintness, resulting in enormous radio-to-infrared flux density ratios of up to several t...

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Bibliographic Details
Main Authors: Herzog, A, Norris, RP, Middelberg, E, Seymour, N, Spitler, LR, Emonts, BHC, Franzen, TMO, Hunstead, R, Intema, HT, Marvil, J, Parker, QA, Sirothia, SK, Hurley-Walker, N, Bell, M, Bernardi, G, Bowman, JD, Briggs, F, Cappallo, RJ, Callingham, JR, Deshpande, AA, Dwarakanath, KS, For, B-Q, Greenhill, LJ, Hancock, P, Hazelton, BJ, Hindson, L, Johnston-Hollitt, M, Kapinska, AD, Kaplan, DL, Lenc, E, Lonsdale, CJ, McKinley, B, McWhirter, SR, Mitchell, DA, Morales, MF, Morgan, E, Morgan, J, Oberoi, D, Offringa, A, Ord, SM, Prabu, T, Procopio, P, Shankar, NU, Srivani, KS, Staveley-Smith, L, Subrahmanyan, R, Tingay, SJ, Wayth, RB, Webster, RL, Williams, A, Heywood, I
Format: Journal article
Published: EDP Sciences 2016

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