Source models in gravitational lens system Q2237+0305 and high amplification events

We analyze a reliability of quasar brightness distribution (BD) parameter estimation on the light curves of different images in the system Q2237+0305 observed by OGLE and GLITP groups during High Amplification Events (HAE). We evaluated the source parameters for as small as possible data interval in...

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Bibliographic Details
Main Authors: E. V. Fedorova, A. N. Aleksandrov, V. I. Zhdanov
Format: Article
Language:English
Published: National Aviation University 2004-12-01
Series:Вісник Астрономічної школи
Online Access:http://astro.nau.edu.ua/issues/2004_V.5_Iss.1-2/229.html