Possible identification of the IR counterpart of SGR 1806-20

Details Possible identification of the IR counterpart of SGR 1806-20 Possible identification of the IR counterpart of SGR 1806-20

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..378....1i&link_type=abstract

The Astronomer's Telegram, #378

Astronomy and Astrophysics

Astronomy

5

Infra-Red, Gamma Ray, Soft Gamma-Ray Repeaters

Scientific paper

Following the recent radio detection of SGR 1806-20 (Gaensler et al. 2005, GCN 2929) which provided an unprecedented positional accuracy (at the level of 0.1"), we re-analysed all the VLT NACO images of the field (in J, H and Ks bands) we collected in 2004 after the X-ray burst activity from the source detected during March, June, August and October 2004.

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