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The Robotic Optical Transient Search Experiment (ROTSE) is a multi-telescope experiment designed to observe the optical afterglow of gamma-ray bursts. The experiment currently consists of four telescopes located in Australia, Namibia, Turkey, and at the McDonald Observatory near Fort Davis, Texas.[1]
The Namibian telescope is located at the High Energy Stereoscopic System site in the Gamsberg mountains south-west of the capital Windhoek.[1]
The ROTSE project is a collaboration of astrophysicists from the University of Michigan, Los Alamos National Laboratory, Lawrence Livermore National Laboratory, the University of New South Wales (Australia) and the Max Planck Institute for Nuclear Physics (Germany).[2]
The original ROTSE-I had 4 telephoto lenses of 11 cm aperture, covering a 16x16 degree field of view. This detected the first afterglow of a GRB while the burst was still ongoing, but this was the only burst detected by ROTSE or the very similar Livermore Optical Transient Imaging System. Therefore, ROTSE-II was designed, also featuring a large field of view, but it was never built, since new satellites such as HETE-2 and SWIFT could provide smaller error boxes, making a huge field of view unnecessary. This led to the design of ROTSE-III, a more or less conventional telescope designed for fast slewing and operation at multiple locations around the world.[3]
See also
- Super-LOTIS
- List of astronomical observatories
References
- "ROTSE-III World Distribution". Retrieved 11 September 2010.
- "Project Information". Retrieved 11 September 2010.
- Akerlof, C.W. and Ashley, MCB and Casperson, DE and Epps, HW and Kehoe, RL and Marshall, SL and McGowan, KE and McKay, TA and Phillips, MA and Rykoff, E.S.; et al. (2002). "The ROTSE-III robotic telescope system". Publications of the Astronomical Society of the Pacific. 115 (803): 132–140. arXiv:astro-ph/0210238. Bibcode:2003PASP..115..132A. doi:10.1086/345490. S2CID 10152025.
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External links
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На других языках
- [en] Robotic Optical Transient Search Experiment
[ru] ROTSE
ROTSE — астрономический проект, основанный в 1998 году в Лос-Аламосе, Нью-Мексико, США. Название проекта (англ. Robotic Optical Transient Search Experiment) переводится как Эксперимент по роботизированному поиску оптических транзиентов. Проект состоит из множества телескопов малого и среднего размера. Основной целью проекта является обнаружение оптических послесвечений гамма-всплесков.Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.
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