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VLBI20-30: a scientific roadmap for the next decade -- The future of the European VLBI Network | Tiziana Venturi
; Zsolt Paragi
; Michael Lindqvist
; Anna Bartkiewicz
; Rob Beswick
; Tamara Bogdanović
; Walter Brisken
; Patrick Charlot
; Francisco Colomer
; John Conway
; Sándor Frey
; José Carlos Guirado
; Leonid Gurvits
; Huib van Langevelde
; Andrei Lobanov
; John McKean
; Raffaella Morganti
; Tom Muxlow
; Miguel Pérez-Torres
; Kazi Rygl
; Robert Schulz
; Arpad Szomoru
; Pablo de Vicente
; Tao An
; Guillem Anglada
; Megan Argo
; Rebecca Azulay
; Ilse van Bemmel
; Tatiana Bocanegra
; Biagina Boccardi
; Paola Castangia
; James Chibueze
; Giuseppe Cimò
; Juan-Bautista Climent
; Roger Deane
; Adam Deller
; Richard Dodson
; Dmitry Duev
; Sandra Etoka
; Danielle Fenech
; Krisztina Gabányi
; Denise Gabuzda
; Michael Garrett
; Marcin Gawroński
; Giancarlo Ghirlanda
; Marcello Giroletti
; Ciriaco Goddi
; Jose Luis Gómez
; Malcolm Gray
; Jane Greaves
; Jason Hessels
; Alexander van der Horst
; Todd Hunter
; Robert Laing
; Dharam Vir Lal
; Sébastien Lambert
; Laurent Loinard
; Benito Marcote
; Andrea Merloni
; Guifré Molera Calvés
; Luca Moscadelli
; Tom Muxlow
; Hans Olofsson
; Leonid Petrov
; Roberto Pizzo
; Andrea Possenti
; Luis Henry Quiroga-Nuñez
; Cormac Reynolds
; Anita Richards
; Maria Rioja
; Alberto Sanna
; Tuomas Savolainen
; Tullia Sbarrato
; Cristiana Spingola
; Gabriele Surcis
; Corrado Trigilio
; Eskil Varenius
; Wouter Vlemmings
; Sjoert van Velzen
; Johan van der Walt
; | Date: |
5 Jul 2020 | Abstract: | This white paper describes the science case for Very Long Baseline
Interferometry (VLBI) and provides suggestions towards upgrade paths for the
European VLBI Network (EVN). The EVN is a distributed long-baseline radio
interferometric array, that operates at the very forefront of astronomical
research. Recent results, together with the new science possibilities outlined
in this vision document, demonstrate the EVN’s potential to generate new and
exciting results that will transform our view of the cosmos. Together with
e-MERLIN, the EVN provides a range of baseline lengths that permit unique
studies of faint radio sources to be made over a wide range of spatial scales.
The science cases are reviewed in six chapters that cover the following broad
areas: cosmology, galaxy formation and evolution, innermost regions of active
galactic nuclei, explosive phenomena and transients, stars and stellar masers
in the Milky Way, celestial reference frames and space applications. The
document concludes with identifying the synergies with other radio, as well as
multi-band/multi-messenger instruments, and provide the recommendations for
future improvements. The appendices briefly describe other radio VLBI arrays,
the technological framework for EVN developments, and a selection of spectral
lines of astrophysical interest below 100 GHz. The document includes a glossary
for non-specialists, and a list of acronyms at the end. | Source: | arXiv, 2007.2347 | Services: | Forum | Review | PDF | Favorites |
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