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Swift X-Ray Telescope and Very Large Telescope Observations of the Afterglow of GRB 041223

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Published 2005 March 9 © 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation D. N. Burrows et al 2005 ApJ 622 L85 DOI 10.1086/429666

1538-4357/622/2/L85

Abstract

GRB 041223 was the first gamma-ray burst detected by the Swift X-Ray Telescope (XRT), beginning 4.6 hr after the burst. The X-ray detection triggered a VLT observation of the optical/near-infrared (NIR) counterpart, located about 1farcs1 from the XRT position. The X-ray counterpart faded rapidly, with a power-law index of -1.72 ± 0.20, with an average unabsorbed X-ray flux of 6.5 × 10-12 ergs cm-2 s-1 in the 0.5-10 keV band for a power-law spectrum of photon index 2.02 ± 0.13 with Galactic absorption. The NIR counterpart was observed at three epochs between 16 and 87 hr after the burst and faded with a power-law index of -1.14 ± 0.08 with a reddening-corrected spectral energy distribution power-law slope of -0.40 ± 0.03. We find that the X-ray and NIR data are consistent with a two-component jet in a wind medium.

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10.1086/429666