%0 Generic %1 citeulike:14124234 %A Gogus, Ersin %A Lin, Lin %A Kaneko, Yuki %A Kouveliotou, Chryssa %A Watts, Anna L. %A Alpar, M. Ali %A Huppenkothen, Daniela %A Roberts, Oliver J. %A Younes, George %A van der Horst, Alexander J. %D 2016 %K imported %T Magnetar Behavior of a Rotation Powered Pulsar, PSR J1119-6127 %U http://arxiv.org/abs/1608.07133 %X Two energetic hard X-ray bursts have recently triggered the Fermi and Swift space observatories from the rotation powered pulsar, PSR J1119-6127. We have performed in depth spectral and temporal analyses of these two events. Our extensive searches in both observatory data for lower luminosity, untriggered, bursts using two independent methods (a signal-to-noise ratio search and a Bayesian blocks based technique), uncovered 10 additional events from the source. We report here on the timing and energetics of the 12 bursts from PSR J1119-6127 during its burst active phase of 2016 July 26 and 28. We also found a softer, extended thermal burst tail emission, which shows evidence of cooling. We discuss here the implications of these results on the nature of this unusual high-field radio pulsar, which firmly place it within the typical magnetar population.

@misc{citeulike:14124234, abstract = {{Two energetic hard X-ray bursts have recently triggered the Fermi and Swift space observatories from the rotation powered pulsar, PSR J1119-6127. We have performed in depth spectral and temporal analyses of these two events. Our extensive searches in both observatory data for lower luminosity, untriggered, bursts using two independent methods (a signal-to-noise ratio search and a Bayesian blocks based technique), uncovered 10 additional events from the source. We report here on the timing and energetics of the 12 bursts from PSR J1119-6127 during its burst active phase of 2016 July 26 and 28. We also found a softer, extended thermal burst tail emission, which shows evidence of cooling. We discuss here the implications of these results on the nature of this unusual high-field radio pulsar, which firmly place it within the typical magnetar population.}}, added-at = {2019-03-25T08:20:55.000+0100}, archiveprefix = {arXiv}, author = {Gogus, Ersin and Lin, Lin and Kaneko, Yuki and Kouveliotou, Chryssa and Watts, Anna L. and Alpar, M. Ali and Huppenkothen, Daniela and Roberts, Oliver J. and Younes, George and van der Horst, Alexander J.}, biburl = {https://www.bibsonomy.org/bibtex/2b87d84bfe8e23a5cd88dfc2d4cf1c8f1/ericblackman}, citeulike-article-id = {14124234}, citeulike-linkout-0 = {http://arxiv.org/abs/1608.07133}, citeulike-linkout-1 = {http://arxiv.org/pdf/1608.07133}, day = 25, eprint = {1608.07133}, interhash = {3eabda1d1ceb605afceaa0d0e30bdcb4}, intrahash = {b87d84bfe8e23a5cd88dfc2d4cf1c8f1}, keywords = {imported}, month = aug, posted-at = {2016-08-26 22:17:50}, priority = {2}, timestamp = {2019-03-25T08:20:55.000+0100}, title = {{Magnetar Behavior of a Rotation Powered Pulsar, PSR J1119-6127}}, url = {http://arxiv.org/abs/1608.07133}, year = 2016 }