Radio Detection of SGR 1806-20 Following a Giant Flare

Details Radio Detection of SGR 1806-20 Following a Giant Flare Radio Detection of SGR 1806-20 Following a Giant Flare

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..373....1g&link_type=abstract

The Astronomer's Telegram, #373

Astronomy and Astrophysics

Astronomy

2

Neutron Stars, Pulsars, Soft Gamma-Ray Repeaters, Transients, Variables

Scientific paper

We observed the soft gamma-ray repeater SGR 1806-20 with the Very Large Array, approximately 7 days after the detection of a Giant Flare from the source (Borkowski, J. et al., 2004, GCN # 2920), on January 3, 2005 for one hour (19:46-20:46 UT). At frequencies of 1.4, 4.9 and 8.5 GHz, we detect an unresolved radio source at coordinates (J2000) RA 18h08m39.3s, Dec -20o24'39.7", with an approximate uncertainty of 0.1" in each coordinate.

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