Pith. sign in

REVIEW 3 cited by

The SFXC software correlator for Very Long Baseline Interferometry: Algorithms and Implementation

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1502.00467 v1 pith:USJ2E75H submitted 2015-02-02 astro-ph.IM

The SFXC software correlator for Very Long Baseline Interferometry: Algorithms and Implementation

classification astro-ph.IM
keywords softwarecorrelatorcorrelationsfxcvlbialgorithmalgorithmsarchitecture
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

In this paper a description is given of the SFXC software correlator, developed and maintained at the Joint Institute for VLBI in Europe (JIVE). The software is designed to run on generic Linux-based computing clusters. The correlation algorithm is explained in detail, as are some of the novel modes that software correlation has enabled, such as wide-field VLBI imaging through the use of multiple phase centres and pulsar gating and binning. This is followed by an overview of the software architecture. Finally, the performance of the correlator as a function of number of CPU cores, telescopes and spectral channels is shown.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. A Jet from a Nearly Dormant Black Hole

    astro-ph.HE 2026-06 unverdicted novelty 8.0

    Multi-frequency VLBI observations detect a two-sided jet with steep synchrotron spectrum from the nearly dormant SMBH in M60, with frequency-dependent core shift locating the engine ~10 Schwarzschild radii upstream of...

  2. Detection of a parsec-scale, compact, and fading ejecta from an accreting massive black hole

    astro-ph.HE 2026-06 unverdicted novelty 7.0

    VLBI at 4.9 GHz plus multi-epoch survey data reveal a fading parsec-scale radio component near the optical center of a dwarf galaxy, interpreted as transient ejecta from IMBH accretion.

  3. Searching for links between energetic millisecond pulsars and repeating fast radio bursts

    astro-ph.HE 2026-05 unverdicted novelty 4.0

    Wideband observations show M28A giant pulses differ from FRB 20200120E bursts in duration, luminosity, timing statistics, and spectral structure, yielding no strong evidence for a direct link.