The radio spectral energy distribution of infrared-faint radio sources

The radio spectral energy distribution of infrared-faint radio sources

Context: 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 thousand. Aims: Because of thei...

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Main Authors: Herzog, A., Norris, R., Middelberg, E., Seymour, Nick, Spitler, L., Emonts, B., Franzen, T., Hunstead, R., Intema, H., Marvil, J., Parker, Q., Sirothia, S., Hurley-Walker, Natasha, Bell, M., Bernardi, G., Bowman, J., Briggs, F., Cappallo, R., Callingham, J., Deshpande, A., Dwarakanath, K., For, B., Greenhill, L., Hancock, Paul, Hazelton, B., Hindson, L., Johnston-Hollitt, M., Kapińska, A., Kaplan, D., Lenc, E., Lonsdale, C., McKinley, B., McWhirter, S., Mitchell, D., Morales, M., Morgan, E., Morgan, J., Oberoi, D., Offringa, A., Ord, S., Prabu, T., Procopio, P., Udaya Shankar, N., Srivani, K., Staveley-Smith, L., Subrahmanyan, R., Tingay, Steven, Wayth, Randall, Webster, R., Williams, A., Williams, C., Wu, C., Zheng, Q., Bannister, K., Chippendale, A., Harvey-Smith, L., Heywood, I., Indermuehle, B., Popping, A., Sault, R., Whiting, M.
Format: Journal Article
Published: EDP Sciences 2016
Online Access:http://hdl.handle.net/20.500.11937/37438

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