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From truck to optical fibre: the coming-of-age of eVLBI

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arxiv astro-ph/0412686 v1 pith:GNYM4TJG submitted 2004-12-30 astro-ph

classification astro-ph
keywords willreal-timebandwidthcorrelationcorrelatorcurrentdevelopmentevlbi
verification ladder T0 review T1 audit T2 compute T3 formal
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Spurred by the advent of disk-based recording systems and the nearly explosive increase of internet bandwidth, eVLBI (Parsley et al. 2004) has undergone a remarkable development over the past two years. From ftp-based transfers of small amounts of astronomical data, through near real-time correlation (disk-buffered at the correlator), it has culminated this spring in the first three telescope real-time correlation at JIVE (Onsala, Westerbork and Jodrell Bank). In this paper we will give a review of this development and the current state of affairs. We will also address the current limitations and the way we may improve both bandwidth and reliability and finally we will discuss the opportunities a true high-bandwidth real-time VLBI correlator will provide.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 4 citations worldwide. Full citation record

  1. An Ejection Event Captured by VLBI During the Outburst of Swift J1727.8$-$1613

    astro-ph.HE 2025-06 conditional novelty 5.0 of 10

    A 6-hour VLBI observation of Swift J1727.8-1613 reveals a fast-moving radio blob or pair of symmetric blobs, indicating a discrete ejection event during a state transition.

  2. Radiation Pressure Instability in the "turn-on" Changing-Look AGN SDSS J1430+2303

    astro-ph.GA 2026-06 unverdicted novelty 4.0 of 10

    Multi-wavelength data from SDSS J1430+2303 are interpreted as evidence that radiation pressure instabilities drive a shrinking unstable accretion-disk zone, based on timing analysis, weak soft excess, and SED-derived ...

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