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First hours of the GRB 030329 optical afterglow

R. A. Burenin·R. A. Sunyaev·M. N. Pavlinsky·D. V. Denissenko·O. V. Terekhov·A. Yu. Tkachenko·Z. Aslan·I. Khamitov·K. Uluc·M. A. Alpar·U. Kiziloglu·A. Baykal·I. Bikmaev·N. Sakhibullin·V. Suleymanov
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Abstract

We present the first results of the observations of the extremely bright optical afterglow of gamma-ray burst (GRB) 030329 with the 1.5m Russian-Turkish telescope RTT150 (TUBITAK National Observatory, Bakyrlytepe, Turkey). RTT150 was one of the first 1.5m-class telescopes pointed to the afterglow. Observations were started approximately 6 hours after the burst. During the first 5 hours of our observations the afterglow faded exactly as a power law with index -1.19+-0.01 in each of the BVRI Bessel filters. After that, in all BVRI filters simultaneously we observe a steepening of the power law light curve. The power law decay index smoothly approaches the value ~= -1.9, observed by other observatories later. This power law break occurs at t-t_0 =0.57 days and lasts for +-0.1 days. We observe no variability above the gradual fading with the upper limits 10--1% on time scales 0.1--1000s. Spectral flux distribution in four BVRI filters corresponds to the power law spectrum with spectral index α=0.66+-0.01. The change of the power law decay index in the end of our observations can be interpreted as a signature of collimated ultrarelativistic jet. The afterglow flux distribution in radio, optical and x-rays is consistent with synchrotron spectrum. We continue our observations of this unique object with RTT150.

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R. A. Burenin, R. A. Sunyaev, M. N. Pavlinsky, D. V. Denissenko, O. V. Terekhov, A. Yu. Tkachenko, Z. Aslan, I. Khamitov, K. Uluc, M. A. Alpar, U. Kiziloglu, A. Baykal, I. Bikmaev, N. Sakhibullin, V. Suleymanov. 2003-08-01. First hours of the GRB 030329 optical afterglow. https://doi.org/10.1134/1.1607494

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