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Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

Autor: Andreoni, I., Ackley, K., Cooke, J., Acharyya, A., Allison, J. R., Anderson, G. E., Ashley, M. C. B., Baade, D., Bailes, M., Bannister, K., Beardsley, A., Bessell, M. S., Bian, F., Bland, P. A., Boer, M., Booler, T., Brandeker, A., Brown, I. S., Buckley, D., Chang, S. -W., Coward, D. M., Crawford, S., Crisp, H., Crosse, B., Cucchiara, A., Cupák, M., de Gois, J. S., Deller, A., Devillepoix, H. A. R., Dobie, D., Elmer, E., Emrich, D., Farah, W., Farrell, T. J., Franzen, T., Gaensler, B. M., Galloway, D. K., Gendre, B., Giblin, T., Goobar, A., Green, J., Hancock, P. J., Hartig, B. A. D., Howell, E. J., Horsley, L., Hotan, A., Howie, R. M., Hu, L., Hu, Y., James, C. W., Johnston, S., Johnston-Hollitt, M., Kaplan, D. L., Kasliwal, M., Keane, E. F., Kenney, D., Klotz, A., Lau, R., Laugier, R., Lenc, E., Li, X., Liang, E., Lidman, C., Luvaul, L. C., Lynch, C., Ma, B., Macpherson, D., Mao, J., McClelland, D. E., McCully, C., Möller, A., Morales, M. F., Morris, D., Murphy, T., Noysena, K., Onken, C. A., Orange, N. B., Oslowski, S., Pallot, D., Paxman, J., Potter, S. B., Pritchard, T., Raja, W., Ridden-Harper, R., Romero-Colmenero, E., Sadler, E. M., Sansom, E. K., Scalzo, R. A., Schmidt, B. P., Scott, S. M., Seghouani, N., Shang, Z., Shannon, R. M., Shao, L., Shara, M. M., Sharp, R., Sokolowski, M., Sollerman, J., Staff, J., Steele, K., Sun, T., Suntzeff, N. B., Tao, C., Tingay, S., Towner, M. C., Thierry, P., Trott, C., Tucker, B. E., Väisänen, P., Krishnan, V. Venkatraman, Walker, M., Wang, L., Wang, X., Wayth, R., Whiting, M., Williams, A., Williams, T., Wolf, C., Wu, C., Wu, X., Yang, J., Yuan, X., Zhang, H., Zhou, J., Zovaro, H.

The discovery of the first electromagnetic counterpart to a gravitational wave signal has generated follow-up observations by over 50 facilities world-wide, ushering in the new era of multi-messenger astronomy. In this paper, we present follow-up obs

Externí odkaz: http://arxiv.org/abs/1710.05846