Kiso observations for 20 GRBs in HETE-2 era

Details Kiso observations for 20 GRBs in HETE-2 era Kiso observations for 20 GRBs in HETE-2 era

2005-06-10

arxiv.org/abs/astro-ph/0506235v1

Nuovo Cim.C28:779-782,2005

Astronomy and Astrophysics

Astrophysics

5 pages, 4 figure. Accepted for publication into "il nuovo cimento". Proceeding of the 4th Rome GRB conference, eds. L. Piro,

Scientific paper

10.1393/ncc/i2005-10152-y

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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