%0 Generic %1 citeulike:14130104 %A Huege, Tim %A Bray, Justin D. %A Buitink, Stijn %A Butler, David %A Dallier, Richard %A Ekers, Ron D. %A Enßlin, Torsten %A Falcke, Heino %A Haungs, Andreas %A James, Clancy W. %A Martin, Lilian %A Mitra, Pragati %A Mulrey, Katharine %A Revenu, Benoît %A Scholten, Olaf %A Schröder, Frank G. %A Tingay, Steven %A Winchen, Tobias %A Zilles, Anne %D 2016 %K imported %T Ultimate precision in cosmic-ray radio detection &\#45;&\#45;- the SKA %U http://arxiv.org/abs/1608.08869 %X As of 2023, the low-frequency part of the Square Kilometre Array will go online in Australia. It will constitute the largest and most powerful low-frequency radio-astronomical observatory to date, and will facilitate a rich science programme in astronomy and astrophysics. With modest engineering changes, it will also be able to measure cosmic rays via the radio emission from extensive air showers. The extreme antenna density and the homogeneous coverage provided by more than 60,000 antennas within an area of one km\$^2\$ will push radio detection of cosmic rays in the energy range around 10\$^17\$ eV to ultimate precision, with superior capabilities in the reconstruction of arrival direction, energy, and an expected depth-of-shower-maximum resolution of 6\~g/cm\$^2\$.

@misc{citeulike:14130104, abstract = {As of 2023, the low-frequency part of the Square Kilometre Array will go online in Australia. It will constitute the largest and most powerful low-frequency radio-astronomical observatory to date, and will facilitate a rich science programme in astronomy and astrophysics. With modest engineering changes, it will also be able to measure cosmic rays via the radio emission from extensive air showers. The extreme antenna density and the homogeneous coverage provided by more than 60,000 antennas within an area of one km\$^2\$ will push radio detection of cosmic rays in the energy range around 10\$^{17}\$ eV to ultimate precision, with superior capabilities in the reconstruction of arrival direction, energy, and an expected depth-of-shower-maximum resolution of 6\~{}g/cm\${^2}\$.}, added-at = {2019-03-25T08:20:55.000+0100}, archiveprefix = {arXiv}, author = {Huege, Tim and Bray, Justin D. and Buitink, Stijn and Butler, David and Dallier, Richard and Ekers, Ron D. and En{\ss}lin, Torsten and Falcke, Heino and Haungs, Andreas and James, Clancy W. and Martin, Lilian and Mitra, Pragati and Mulrey, Katharine and Revenu, Beno\^{i}t and Scholten, Olaf and Schr\"{o}der, Frank G. and Tingay, Steven and Winchen, Tobias and Zilles, Anne}, biburl = {https://www.bibsonomy.org/bibtex/25d0659b36251d1e72653af018a4c083d/ericblackman}, citeulike-article-id = {14130104}, citeulike-linkout-0 = {http://arxiv.org/abs/1608.08869}, citeulike-linkout-1 = {http://arxiv.org/pdf/1608.08869}, day = 31, eprint = {1608.08869}, interhash = {970c7524d1707c76179fe9606d04a88d}, intrahash = {5d0659b36251d1e72653af018a4c083d}, keywords = {imported}, month = aug, posted-at = {2016-09-05 05:45:28}, priority = {2}, timestamp = {2019-03-25T08:20:55.000+0100}, title = {{Ultimate precision in cosmic-ray radio detection \&\#45;\&\#45;- the SKA}}, url = {http://arxiv.org/abs/1608.08869}, year = 2016 }