TY - JOUR
T1 - From TORTORA to MegaTORTORA-results and prospects of search for fast optical transients
AU - Beskin, Grigory
AU - Bondar, Sergey
AU - Karpov, Sergey
AU - Plokhotnichenko, Vladimir
AU - Guarnieri, Adriano
AU - Bartolini, Corrado
AU - Greco, Giuseppe
AU - Piccioni, Adalberto
AU - Shearer, Andrew
PY - 2010
Y1 - 2010
N2 - To study short stochastic optical flares of different objects (GRBs, SNs, etc.) of unknown localizations as well as NEOs it is necessary to monitor large regions of sky with high-time resolution. We developed a system consisting of widefield camera with field of view of 400600 sq.deg. which uses TV-CCD with 0.13s temporal resolution to record and classify optical transients, and a fast robotic telescope aimed to perform their spectroscopic and photometric investigation just after detection. Such two-telescope complex, combining wide-field camera TORTORA and robotic telescope REM, operated from May 2006 at La Silla ESO observatory. Some results of its operation, including first high time resolution study of optical transient accompanying GRB and discovery of its fine time structure, are presented. Also, prospects for improving the efficiency of such observations are given, and a project of a next generation wide field monitoring system, the MegaTORTORA, is described.
AB - To study short stochastic optical flares of different objects (GRBs, SNs, etc.) of unknown localizations as well as NEOs it is necessary to monitor large regions of sky with high-time resolution. We developed a system consisting of widefield camera with field of view of 400600 sq.deg. which uses TV-CCD with 0.13s temporal resolution to record and classify optical transients, and a fast robotic telescope aimed to perform their spectroscopic and photometric investigation just after detection. Such two-telescope complex, combining wide-field camera TORTORA and robotic telescope REM, operated from May 2006 at La Silla ESO observatory. Some results of its operation, including first high time resolution study of optical transient accompanying GRB and discovery of its fine time structure, are presented. Also, prospects for improving the efficiency of such observations are given, and a project of a next generation wide field monitoring system, the MegaTORTORA, is described.
UR - https://www.scopus.com/pages/publications/78349240112
U2 - 10.1155/2010/171569
DO - 10.1155/2010/171569
M3 - Article
SN - 1687-7969
VL - 2010
JO - Advances in Astronomy
JF - Advances in Astronomy
M1 - 171569
ER -