13-19 March 2016
Africa/Johannesburg timezone
<a href="http://events.saip.org.za/internalPage.py?pageId=12&confId=56">Proceedings, </a> <a href="http://events.saip.org.za/materialDisplay.py?materialId=4&confId=56"> Programme and Book of Abstracts</a> and <a href="http://events.saip.org.za/getFile.py/access?resId=1&materialId=4&confId=56">Errata</a>

The impact of the broadband VLBI on the next decade

14 Mar 2016, 15:45
1h
Board: S1P4
Poster Presentation 1: Advances in VGOS Stations and Technology Poster1-3

Speakers

Dr Kazuhiro Takefuji (NICT) Dr Mamoru Sekido (National Institute of Information and Communications Technology)

Description

The Kashima 34 m radio telescope, the cassegrain optics is currently realized 3.2GHz to 14 GHz receiver system by installing the NINJA feed. Furthermore a direct sampler GALAS easily connect four 1GHz bandwidth without any analogue frequency converter and phase-cal. VGOS, EHT and other astronomy VLBI highly demand broadband system for better delay determination, shorter integration time and better SNR. We will report our progress of developing broadband system and recent results.

Primary author

Co-author

Dr Mamoru Sekido (National Institute of Information and Communications Technology)

Presentation Materials

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