Upper limit on the radio emission from the soft gamma-ray repeater SGR 1833-0832

Details Upper limit on the radio emission from the soft gamma-ray repeater SGR 1833-0832 Upper limit on the radio emission from the soft gamma-ray repeater SGR 1833-0832

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2515....1b&link_type=abstract

The Astronomer's Telegram, #2515

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2

Radio, Pulsars, Supernova Remnants

Scientific paper

The soft gamma-ray repeater J1833-0832 has been discovered on 2010 March 19 thanks to the detection of a short burst by Swift (GCN #10526). Prompted by the detection of a radio outburst following the X-ray transient activity of two other magnetars, the anomalous X-ray pulsars XTE J1810-197 and 1E 1547.0-5408 (Camilo et al. 2006, Nature, 442, 892; 2007, ApJ, 666, L93), we observed the source with the 64-m Parkes radio telescope.

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