arxiv: astro-ph/0506235 · v1 · pith:3WE3DZRKnew · submitted 2005-06-10 · 🌌 astro-ph

Kiso observations for 20 GRBs in HETE-2 era

Y. Urata , Y. Nakada , T. Miyata , T. Aoki , T. Soyano , K. Tarusawa , H. Mito , S. Nishiura

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T. Tamagawa K. Makishima

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classification 🌌 astro-ph

keywords follow-upsystemkisoobservationsafterglowsbeenearlyhete-2

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We have established a GRB follow-up observation system at Kiso observatory (Japan) in 2001. Since the east Asian area had been blank for the GRB follow-up observational network, this observational system is very important in studying the temporal and spectral evolution of early afterglows. Using this system, we have performed quick observations for optical afterglows from early phase based on HETE-2 and INTEGRAL alerts. Thanks to the quick follow-up observation system, we have been able to use the Kiso observatory in 20 events, and conduct their follow-up observations in optical and near infrared wavelengths.

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Kiso observations for 20 GRBs in HETE-2 era

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