对RT-22在18-26 GHz频段采用连续频率合成方法的结果

2014 24th International Crimean Conference Microwave & Telecommunication Technology Pub Date : 2014-11-20 DOI:10.1109/CRMICO.2014.6959777

L. Volvach, A. Volvach, M. Larionov, V. Kostenko, I. Litovchenko

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引用次数: 0

摘要

介绍了在“Radioastron”项目框架下，RT-22 (Simeiz)和RT-70 (Yevpatoriya)在18-26 GHz连续频率合成方法下的VLBI观测结果。确定了5个活动星系核(BL Lac、2145+067、3C454.3、3C84、0528+134)和水蒸汽线2个源(W3OH和ORION KL)的相互关联函数。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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Results of using the method of successive frequency synthesis on RT-22 at 18–26 GHz

The results of VLBI observations between the RT-22 (Simeiz) and RT-70 (Yevpatoriya) using the method of successive frequency synthesis at 18-26 GHz within the framework of “Radioastron” project are presented. The cross-correlation functions for five active galactic nuclei (BL Lac, 2145+067, 3C454.3, 3C84, 0528+134) and two sources in water vapor line (W3OH and ORION KL) are determined.

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2014 24th International Crimean Conference Microwave & Telecommunication Technology

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