For, B., Staveley-Smith, L., Hurley-Walker, N., Franzen, T., Kapińska, A. D., Filipović, M. D., Collier, J. D., Wu, C., Grieve, K., Callingham, J. R., Bell, M. E., Bernardi, G., Bowman, J. D., Briggs, F., Cappallo, R. J., Deshpande, A. A., Dwarakanath, K. S., Gaensler, B. M., Greenhill, L. J., Hancock, P., Hazelton, B. J., Hindson, L., Johnston-Hollitt, M., Kaplan, D. L., Lenc, E., Lonsdale, C. J., McKinley, B., McWhirter, S. R., Mitchell, D. A., Morales, M. F., Morgan, E., Morgan, J., Oberoi, D., Offringa, A., Ord, S. M., Prabu, T., Procopio, P., Shankar, N. U., Srivani, K. S., Subrahmanyan, R., Tingay, S. J., Wayth, R. B., Webster, R. L., Williams, A., Williams, C. L., & Zheng, Q. (2018). a multifrequency radio continuum study of the Magellanic Clouds – I. Overall structure and star formation rates. Monthly notices of the Royal Astronomical Society, 480(2), 2743–2756. http://access.bl.uk/ark:/81055/vdc_100116602853.0x000049