BRAND - The next generation receiver for VLBI
Paper i proceeding, 2018

The aim of the BRAND EVN project is to build a very wide receiver prototype for primary focus with a frequency range from 1.5 GHz to 15.5 GHz In addition we will investigate solutions for secondary focus telescopes. The project has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 730562 [RadioNet]. We present the status of the project which was started on January 1st, 2017 and is progressing smoothly: Feed, LNA, filters, major digital components, and some of the firmware are available now. © Copyright owned by the author(s) under the terms of the Creative Commons.

Författare

Walter Alef

Max-Planck-Gesellschaft

Gino Tuccari

Max-Planck-Gesellschaft

Istituto nazionale di astrofisica (INAF)

S. Dornbusch

Max-Planck-Gesellschaft

M. Wunderlich

Max-Planck-Gesellschaft

Miroslav Pantaleev

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium, Elektroniklaboratorium

Jonas Flygare

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium, Rymdgeodesi och geodynamik

J. D. Gallego

Observatorio de Yebes (IGN)

J. Lopez Perez

Observatorio de Yebes (IGN)

F. Tercero

Observatorio de Yebes (IGN)

G. Schoonderbeek

Netherlands Institute for Radio Astronomy (ASTRON)

J. Hargreaves

Netherlands Institute for Radio Astronomy (ASTRON)

R. de Wild

Netherlands Institute for Radio Astronomy (ASTRON)

V. Bezrukovs

Ventspils Augstskolas

Proceedings of Science

18248039 (eISSN)

Vol. 344

14th European VLBI Network Symposium and Users Meeting, EVN 2018
Granada, Spain,

Infrastruktur

Onsala rymdobservatorium

Ämneskategorier

Signalbehandling

Annan elektroteknik och elektronik

DOI

10.22323/1.344.0081

Mer information

Senast uppdaterat

2020-04-30