Pulsar Astrometry by Using VLBl (PSR0329 between Kashima 26mo & Usuda 64mo)

Abstract

Communications Research Laboratory (CRL), carried out and VLBi (Very Long Baseline Interferometer) experiment of the pulsar 0329 + 54 on November in 1992 between Kashima 26md and Usuda 64md. We got a correlation for it by using K-3 VLBi correlator, which was developed by CRL. Though we observed a slow pulsar this time, we are going to make millisecond pulsar experiments by making good use of this result and by using K-4 correlator which is under developing in CRL. Its result will give us precise positions and proper motions of pulsars which are useful for obtaining precise pulsar timing.

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Document Details

Document Type
Technical Report
Publication Date
Dec 01, 1992
Accession Number
ADA519417

Entities

People

  • H. Hirabayashi
  • H. Kiuchi
  • H. Kobayashi
  • K. Fujlsawa
  • M. Imae
  • S. Hama
  • Y. Hanado
  • Y. Takahshi

Tags

DTIC Thesaurus Topics

  • Abstracts
  • Availability
  • Classification
  • Clocks
  • Contracts
  • Correlators
  • Information Operations
  • Instructions
  • Instrumentation
  • Interferometers
  • Intervals
  • Measurement
  • Measuring Instruments
  • Monitoring
  • Security
  • Time Intervals

Fields of Study

  • Physics

Readers

  • Astronomy/Astrophysics
  • Positioning, Navigation, and Timing (PNT) Technology.