Galactic synchrotron emissivity measurements between 250° < l < 355° from the GLEAM survey with the MWA

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Galactic synchrotron emissivity measurements between 250° < l < 355° from the GLEAM survey with the MWA

Synchrotron emission pervades the Galactic plane at low radio frequencies, originating from cosmic ray electrons interacting with the Galactic magnetic field. Using a low-frequency radio telescope, the Murchison Widefield Array (MWA), we measure the free-free absorption of this Galactic synchrotron...

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Bibliographic Details
Main Authors:	Su, H., Hurley-Walker, Natasha, Jackson, Carole, McClure-Griffiths, N., Tingay, Steven, Hindson, L., Hancock, P., Wayth, Randall, Gaensler, B., Staveley-Smith, L., Morgan, J., Johnston-Hollitt, M., Lenc, E., Bell, M., Callingham, J., Dwarkanath, K., For, B., Kapinska, A., McKinley, B., Offringa, A., Procopio, P., Wu, C., Zheng, Q.
Format:	Journal Article
Published:	Oxford University Press 2017
Online Access:	http://hdl.handle.net/20.500.11937/51676

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