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Status and perspectives of Mini-MegaTORTORA wide-fieldmonitoring system with high temporal resolution

Published online by Cambridge University Press:  22 July 2013

S. Karpov
Affiliation:
Special Astrophysical Observatory of Russian Academy of Sciences, Russia
G. Beskin
Affiliation:
Special Astrophysical Observatory of Russian Academy of Sciences, Russia
S. Bondar
Affiliation:
Institute for Precise Instrumentation, Russia
A. Perkov
Affiliation:
Institute for Precise Instrumentation, Russia
E. Ivanov
Affiliation:
Institute for Precise Instrumentation, Russia
A. Guarnieri
Affiliation:
Bologna University, Italy
C. Bartolini
Affiliation:
Bologna University, Italy
G. Greco
Affiliation:
Astronomical Observatory of Bologna, INAF, Italy
A. Shearer
Affiliation:
National University of Ireland, Galway, Ireland
V. Sasyuk
Affiliation:
Kazan Federal University, Kazan, Russia
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Abstract

Here we briefly summarize our long period experience of constructing and operatingwide-field monitoring cameras with sub-second temporal resolution to look for opticalcomponents of GRBs, fast-moving satellites and meteors. General requirements for hardwarefor such systems are discussed along with algorithms of real-time detection andclassification of various kinds of short optical transients. We also give a status reporton the next generation, multi-objective and transforming monitoring system, theMegaTORTORA, whose 6-channel (Mini-MegaTORTORA-Spain) and 9-channelprototypes (Mini-MegaTORTORA-Kazan) we are building now at SAO RAS. This system combines awide field of view with subsecond temporal resolution in monitoring regime, and is able toreconfigure itself, in a fractions of second, to follow-up mode which has bettersensitivity and provides us with multi-color and polarimetric information on detectedtransients simultaneously.

Type
Research Article
Copyright
© EAS, EDP Sciences 2013

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References

Beskin, G., Bad’in, V., Biryukov, A., et al., 2005, Nuovo Cimento C, 28, 751
Beskin, G., Bondar, S., Karpov, S., et al., 2010a, Adv. Astron., 2010
Beskin, G., de-Bur, V., Karpov, S., Plokhotnichenko, V., & Bondar, S., 2007, Bull. Spec. Astrophysical Observatory, 60-61, 217
Beskin, G., Karpov, S., Bondar, S., et al., 2010b, ApJ, 719, L10 CrossRef
Bondi, H., 1970, Q.J.R. Astron. Soc., 11, 443
Karpov, S., Bad’in, D., Beskin, G., et al., 2004, Astron. Nachr., 325, 677 CrossRef
Karpov, S., Beskin, G., Biryukov, A., et al., 2005, Nuovo Cimento C, 28, 747
Molinari, E., Bondar, S., Karpov, S., et al., 2006, Nuovo Cimento B, 121, 1525
Racusin, J.L., Gehrels, N., Holland, S.T., et al., 2008, GRB Coordinates Network Circular, 7427, 1
Schaefer, B., 1985, AJ, 11, 1363 CrossRef
Schaefer, B., 1987, A&A, 174, 338 PubMed
Zolotukhin, I., Beskin, G., Biryukov, A., et al., 2004, Astron. Nachr., 325, 675 CrossRef