SGR 1806-20: X-ray and IR post-Giant Flare monitoring

Details SGR 1806-20: X-ray and IR post-Giant Flare monitoring SGR 1806-20: X-ray and IR post-Giant Flare monitoring

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..645....1r&link_type=abstract

The Astronomer's Telegram, #645

Physics

Optics

9

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

Scientific paper

We report on the status of our IR and X-ray monitoring the SGR 1806-20 after the 2004 December 27th Giant Flare. The IR counterpart of SGR1806-20 (Israel et al. 2005, A&A, 438, L1; Kosugi et al. 2005, ApJ, 623, L125) was observed on 11-12th September 2005 at the VLT-UT4 equipped with the IR adaptive optics instrument NAOS-CONICA in the Ks band (2400s of effective exposure time) under good sky conditions.

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