An analysis of the halo and relic radio emission from Abell 3376 from Murchison widefield array observations

An analysis of the halo and relic radio emission from Abell 3376 from Murchison widefield array observations

We have carried out multiwavelength observations of the nearby (z = 0.046) rich, merging galaxy cluster Abell 3376 with the Murchison Widefield Array (MWA). As a part of the GaLactic and Extragalactic All-sky MWA Survey, this cluster was observed at 88, 118, 154, 188, and 215 MHz. The known radio re...

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Bibliographic Details
Main Authors: George, L., Dwarakanath, K., Johnston-Hollitt, M., Hurley-Walker, N., Hindson, L., Kapinska, A., Tingay, Steven, Bell, M., Callingham, J., For, B., Hancock, P., Lenc, E., McKinley, B., Morgan, J., Offringa, A., Procopio, P., Staveley-Smith, L., Wayth, Randall, Wu, C., Zheng, Q., Bernardi, G., Bowman, J., Briggs, F., Cappallo, R., Corey, B., Deshpande, A., Emrich, D., Goeke, R., Greenhill, L., Hazelton, B., Kaplan, D., Kasper, J., Kratzenberg, E., Lonsdale, C., Lynch, Mervyn, McWhirter, S., Mitchell, D., Morales, M., Morgan, E., Oberoi, D., Ord, S., Prabu, T., Rogers, A., Roshi, A., Udaya Shankar, N., Srivani, K., Subrahmanyan, R., Waterson, M., Webster, R., Whitney, A., Williams, A., Williams, C.
Format: Journal Article
Published: Oxford University Press 2015
Online Access:http://hdl.handle.net/20.500.11937/29898

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