Swift-UVOT captures the earliest ultraviolet spectrum of a Gamma Ray Burst

Details Swift-UVOT captures the earliest ultraviolet spectrum of a Gamma Ray Burst Swift-UVOT captures the earliest ultraviolet spectrum of a Gamma Ray Burst

2008-12-15

arxiv.org/abs/0812.2943v2

Astronomy and Astrophysics

Astrophysics

4 pages, 4 figures, accepted by MNRAS letters

Scientific paper

10.1111/j.1745-3933.2009.00632.x

We present the earliest ever ultraviolet spectrum of a gamma-ray burst (GRB) as observed with the Swift-UVOT. The GRB 081203A spectrum was observed for 50 seconds with the UV grism starting 251 seconds after the Swift-BAT trigger when the GRB was of u ~13.4 mag and still rising to its peak optical brightness. The UV grism spectrum shows a damped Ly-alpha line, Ly-beta, and the Lyman continuum break at a redshift z = 2.05 +/- 0.01. A model fit to the Lyman absorption implies log N(HI) = 22.0 +/- 0.2 cm-2, which is typical for GRB host galaxies with damped Ly-alpha absorbers. This observation of GRB 081203A demonstrates that for GRBs brighter than v ~14 mag and with 0.5 < z < 3.5 the UVOT will be able to provide redshifts, and probe for damped Ly-alpha absorbers within 4-6 minutes from the time of the Swift-BAT trigger.

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