Z. Y. Liu, H. Tong, J. P. Yuan
The magnetar Swift J1834.9-0846 is observed using Nanshan 25 meter radio telescope. No pulsed radio emission is detected. The upper limit on pulsed radio emission from this source is 0.5 mJy. According to the fundamental plane of magnetar radio emissions, this source should have radio emissions. Therefore, our results put constraints on the existence of fundamental plane of magnetar radio emissions. It may be that a small quiescent X-ray luminosity is only a necessary condition for magnetar radio emissions.
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http://arxiv.org/abs/1210.2799
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