Early-time optical spectral shape measurements of GRB 200925B

Zhavlonbek Abdullayev; Toktarkhan Komesh; Bruce Grossan; Ernazar Abdikamalov; Zhanat Maksut; Maxim Krugov; Shynaray Myrzakul; Duriya Tuiakbayeva

arXiv · 2401.09805

Early-time optical spectral shape measurements of GRB 200925B

Zhavlonbek Abdullayev·Toktarkhan Komesh·Bruce Grossan·Ernazar Abdikamalov·Zhanat Maksut·Maxim Krugov·Shynaray Myrzakul·Duriya Tuiakbayeva

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Abstract

Optical broad-band spectral shape measurements of gamma-ray bursts (GRBs) are typically made starting an hour or more after the trigger event. With our automated, rapid-response system, the Burst Simultaneous Three-channel Imager (BSTI) on the Nazarbayev University Transient Telescope at Assy-Turgen Astrophysical Observatory (NUTTelA-TAO), we began measurements of GRB200925B 129 s after the Swift BAT trigger. The temporal decay log slopes in the g', r', and i' bands in the time interval 129 s to 1029 s are -0.43 \pm 0.31, -0.43 \pm 0.15, and -0.72 \pm 0.14, respectively. During the decay phase, a shift in color from red to blue, a change in log slope of \{beta} from -2.73 to -1.52 was measured. The evolution in the optical spectral slope is consistent with a decrease in extinction caused by dust destruction.

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Zhavlonbek Abdullayev, Toktarkhan Komesh, Bruce Grossan, Ernazar Abdikamalov, Zhanat Maksut, Maxim Krugov, Shynaray Myrzakul, Duriya Tuiakbayeva. 2024-01-18. Early-time optical spectral shape measurements of GRB 200925B. https://arxiv.org/abs/2401.09805

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