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CoLiTec software - detection of the near-zero apparent motion

Published online by Cambridge University Press:  30 May 2017

Sergii V. Khlamov ,
Vadym E. Savanevych ,
Olexandr B. Briukhovetskyi  and
Artem V. Pohorelov
Sergii V. Khlamov*
Affiliation:
Kharkiv National University of Radio Electronics, 14 Nauki Ave, Kharkiv UA-61166, Ukraine email: [email protected]
Vadym E. Savanevych*
Affiliation:
Western Radio Technical Surveillance Center, National Space Agency of Ukraine, Kosmonavtiv St, Mukachevo UA-89600, Ukraine email: [email protected]
Olexandr B. Briukhovetskyi
Affiliation:
Western Radio Technical Surveillance Center, National Space Agency of Ukraine, Kosmonavtiv St, Mukachevo UA-89600, Ukraine email: [email protected]
Artem V. Pohorelov
Affiliation:
Kharkiv National University of Radio Electronics, 14 Nauki Ave, Kharkiv UA-61166, Ukraine email: [email protected]
*
†[email protected]
†[email protected]
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Abstract

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In this article we described CoLiTec software for full automated frames processing. CoLiTec software allows processing the Big Data of observation results as well as processing of data that is continuously formed during observation. The scope of solving tasks includes frames brightness equalization, moving objects detection, astrometry, photometry, etc. Along with the high efficiency of Big Data processing CoLiTec software also ensures high accuracy of data measurements. A comparative analysis of the functional characteristics and positional accuracy was performed between CoLiTec and Astrometrica software. The benefits of CoLiTec used with wide field and low quality frames were observed. The efficiency of the CoLiTec software was proved by about 700.000 observations and over 1.500 preliminary discoveries.

Keywords

Methods: analyticaldata analysisnumericalstatisticaltechniques: image processingsurveysastrometrycomets: generalindividual: ISONminor planetsasteroids
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S325: Astroinformatics , October 2016 , pp. 349 - 352
Copyright
Copyright © International Astronomical Union 2017 

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