High-energy sources at low radio frequency: The Murchison Widefield Array view of Fermi blazars

© ESO 2016. Context. Low-frequency radio arrays are opening a new window for the study of the sky, both to study new phenomena and to better characterize known source classes. Being flat-spectrum sources, blazars are so far poorly studied at low radio frequencies. Aims. We characterize the spectral...

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Bibliographic Details
Main Authors: Giroletti, M., Massaro, F., D'Abrusco, R., Lico, R., Burlon, D., Hurley-Walker, Natasha, Johnston-Hollitt, M., Morgan, J., Pavlidou, V., Bell, M., Bernardi, G., Bhat, Ramesh, Bowman, J., Briggs, F., Cappallo, R., Corey, B., Deshpande, A., Ewall-Rice, A., Emrich, David, Gaensler, B., Goeke, R., Greenhill, L., Hazelton, B., Hindson, L., Kaplan, D., Kasper, J., Kratzenberg, E., Feng, L., Jacobs, D., Kudryavtseva, N., Lenc, E., Lonsdale, C., Lynch, Mervyn, McKinley, B., McWhirter, S., Mitchell, D., Morales, M., Morgan, E., Oberoi, D., Offringa, A., Ord, S., Pindor, B., Prabu, T., Procopio, P., Riding, J., Rogers, A., Roshi, A., Udaya Shankar, N., Srivani, K., Subrahmanyan, R., Tingay, Steven, Waterson, M., Wayth, Randall, Webster, R., Whitney, A., Williams, A., Williams, C.
Format: Journal Article
Published: EDP Sciences 2016
Online Access:http://hdl.handle.net/20.500.11937/47810

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