EURO-ASIAN COLLABORATION FOR GAMMA-RAY BURST OPTICAL OBSERVATIONS

Автор(и)

  • A. S. Bogdanov Kalinenkov Astronomical Observatory, Nikolaev State University, Nikolskaya 24, Nikolaev, 54030 Ukraine, Україна
  • S. S. Guziy Kalinenkov Astronomical Observatory, Nikolaev State University, Nikolskaya 24, Nikolaev, 54030 Ukraine, Україна
  • A. J. Castro-Tirado PO Box 3004, 18080 Granada, Spain, Іспанія
  • A. de. Ugarte Postigo PO Box 3004, 18080 Granada, Spain, Іспанія
  • J. Gorosabel PO Box 3004, 18080 Granada, Spain, Іспанія
  • M. Jelinek PO Box 3004, 18080 Granada, Spain, Іспанія
  • V. V. Sokolov Special Astrophysical Observatory of the Russian Academy of Sci. (SAO-RAS) Nizhnij Arkhyz, Karachai-Cirkassian Republic, 369167 Russia, Російська Федерація
  • T. A. Fatkhullin Special Astrophysical Observatory of the Russian Academy of Sci. (SAO-RAS) Nizhnij Arkhyz, Karachai-Cirkassian Republic, 369167 Russia, Російська Федерація
  • I. M. Kheifets Kalinenkov Astronomical Observatory, Nikolaev State University, Nikolskaya 24, Nikolaev, 54030 Ukraine, Україна

DOI:

https://doi.org/10.18524/1810-4215.2007.20.93635

Ключові слова:

gamma rays, bursts - techniques, observations

Анотація

Gamma-ray burst (GRB) very interesting objects in Universe. In the study of gamma-ray burst is very important operative observations with many points in first day and other days after the burst. INTEGRAL, HETE-II and specially SWIFT era is going to leave a considerable number of detections that will allow to do important statistical analysis. We present information about Euro-Asian collaboration for GRB optical observations. To our group included researchers from: Spain, Ukraine, Russia, India, New Zealand and Czech Republic. The instruments which we using for observation have a diameter from 60cm to 6m. Optical and NIR observations are more important.

Посилання

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Опубліковано

2017-03-14

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