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Evaluation of microlens distributions in gravitationally lensed systems based on accurate radio observations

Published online by Cambridge University Press:  26 February 2013

Alexander F. Zakharov ,
Saša Simić ,
Luka Č. Popović  and
Predrag Jovanović
Alexander F. Zakharov*
Affiliation:
Institute of Theoretical and Experimental Physics, Moscow, 117259, Russia Bogoliubov Laboratory of Theoretical Physics, JINR, Dubna, Russia CREST and NASA Research Centers, North Carolina Central University, Durham, NC 27707, USA
Saša Simić
Affiliation:
Faculty of Science, University of Kragujevac, 34000 Kragujevac, Serbia
Luka Č. Popović
Affiliation:
Astronomical Observatory, Volgina 7, Belgrade, 11160, Serbia
Predrag Jovanović
Affiliation:
Faculty of Science, University of Kragujevac, 34000 Kragujevac, Serbia
*
†E-mail: zakharov@itep.ru
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Abstract

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Enormous progress is being made in developing observational facilities. As a result, there are new opportunities to observe structures at sub-mas resolution. To explore gravitationally lensed systems, we simulate radio-lobe images distorted by microlensing. We show that the positions of ‘holes’ in lensed images may indicate the positions of microlens groups or overdensities.

Keywords

gravitational lensing
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S289: Advancing the Physics of Cosmic Distances , August 2012 , pp. 437 - 440
Copyright
Copyright © International Astronomical Union 2013

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