dc.contributor.author |
Karpov S. |
|
dc.contributor.author |
Beskin G. |
|
dc.contributor.author |
Bondar S. |
|
dc.contributor.author |
Perkov A. |
|
dc.contributor.author |
Ivanov E. |
|
dc.contributor.author |
Guarnieri A. |
|
dc.contributor.author |
Bartolini C. |
|
dc.contributor.author |
Greco G. |
|
dc.contributor.author |
Shearer A. |
|
dc.contributor.author |
Sasyuk V. |
|
dc.date.accessioned |
2018-09-18T20:24:09Z |
|
dc.date.available |
2018-09-18T20:24:09Z |
|
dc.date.issued |
2013 |
|
dc.identifier.issn |
1633-4760 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/139509 |
|
dc.description.abstract |
Here we briefly summarize our long period experience of constructing and operating wide-field monitoring cameras with sub-second temporal resolution to look for optical components of GRBs, fast-moving satellites and meteors. General requirements for hardware for such systems are discussed along with algorithms of real-time detection and classification of various kinds of short optical transients. We also give a status report on the next generation, multi-objective and transforming monitoring system, the MegaTORTORA, whose 6-channel (Mini-MegaTORTORA-Spain) and 9-channel prototypes (Mini-MegaTORTORA-Kazan) we are building now at SAO RAS. This system combines a wide field of view with subsecond temporal resolution in monitoring regime, and is able to reconfigure itself, in a fractions of second, to follow-up mode which has better sensitivity and provides us with multi-color and polarimetric information on detected transients simultaneously. © EAS, EDP Sciences 2013. |
|
dc.relation.ispartofseries |
EAS Publications Series |
|
dc.title |
Status and perspectives of Mini-MegaTORTORA wide-field monitoring system with high temporal resolution |
|
dc.type |
Conference Paper |
|
dc.relation.ispartofseries-volume |
61 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
465 |
|
dc.source.id |
SCOPUS16334760-2013-61-SID84887096573 |
|