From TORTORA to MegaTORTORA—Results and Prospects of Search for Fast Optical Transients

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 400–600 sq.deg. which uses TV...

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Main Authors: Grigory Beskin, Sergey Bondar, Sergey Karpov, Vladimir Plokhotnichenko, Adriano Guarnieri, Corrado Bartolini, Giuseppe Greco, Adalberto Piccioni, Andrew Shearer
Format: Article
Language:English
Published: Wiley 2010-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2010/171569
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author Grigory Beskin
Sergey Bondar
Sergey Karpov
Vladimir Plokhotnichenko
Adriano Guarnieri
Corrado Bartolini
Giuseppe Greco
Adalberto Piccioni
Andrew Shearer
author_facet Grigory Beskin
Sergey Bondar
Sergey Karpov
Vladimir Plokhotnichenko
Adriano Guarnieri
Corrado Bartolini
Giuseppe Greco
Adalberto Piccioni
Andrew Shearer
author_sort Grigory Beskin
collection DOAJ
description 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 400–600 sq.deg. which uses TV-CCD with 0.13 s 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.
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series Advances in Astronomy
spelling doaj-art-cca70144d8f94e849c6d32bc086310bc2025-02-03T06:42:16ZengWileyAdvances in Astronomy1687-79691687-79772010-01-01201010.1155/2010/171569171569From TORTORA to MegaTORTORA—Results and Prospects of Search for Fast Optical TransientsGrigory Beskin0Sergey Bondar1Sergey Karpov2Vladimir Plokhotnichenko3Adriano Guarnieri4Corrado Bartolini5Giuseppe Greco6Adalberto Piccioni7Andrew Shearer8Special Astrophysical Observatory of Russian Academy of Sciences, Nizhnij Arkhys 369167, RussiaArkhyz Branch, Institute for Precise Instrumentation, Nizhnij Arkhys 369167, RussiaSpecial Astrophysical Observatory of Russian Academy of Sciences, Nizhnij Arkhys 369167, RussiaSpecial Astrophysical Observatory of Russian Academy of Sciences, Nizhnij Arkhys 369167, RussiaAstronomy Department, Bologna University, 40126 Bologna, ItalyAstronomy Department, Bologna University, 40126 Bologna, ItalyAstronomy Department, Bologna University, 40126 Bologna, ItalyAstronomy Department, Bologna University, 40126 Bologna, ItalySchool of Physics, National University of Ireland, University Road, Galway, IrelandTo 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 400–600 sq.deg. which uses TV-CCD with 0.13 s 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.http://dx.doi.org/10.1155/2010/171569
spellingShingle Grigory Beskin
Sergey Bondar
Sergey Karpov
Vladimir Plokhotnichenko
Adriano Guarnieri
Corrado Bartolini
Giuseppe Greco
Adalberto Piccioni
Andrew Shearer
From TORTORA to MegaTORTORA—Results and Prospects of Search for Fast Optical Transients
Advances in Astronomy
title From TORTORA to MegaTORTORA—Results and Prospects of Search for Fast Optical Transients
title_full From TORTORA to MegaTORTORA—Results and Prospects of Search for Fast Optical Transients
title_fullStr From TORTORA to MegaTORTORA—Results and Prospects of Search for Fast Optical Transients
title_full_unstemmed From TORTORA to MegaTORTORA—Results and Prospects of Search for Fast Optical Transients
title_short From TORTORA to MegaTORTORA—Results and Prospects of Search for Fast Optical Transients
title_sort from tortora to megatortora results and prospects of search for fast optical transients
url http://dx.doi.org/10.1155/2010/171569
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