Peculiarities of Processing VLBI Observations of Pulsars

Details Peculiarities of Processing VLBI Observations of Pulsars Peculiarities of Processing VLBI Observations of Pulsars

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003astl...29...96s&link_type=abstract

Astronomy Letters, vol. 29, p. 96-104 (2003)

Astronomy and Astrophysics

Astronomy

4

Scientific paper

We determined the features of pulsars that were disregarded in standard amplitude-calibration procedures for VLBI observations. We suggest additional amplitude-calibration methods. These methods were used to process the VLBI observations of the pulsar PSR B0329+54 carried out with the HALCA ground-space interferometer. Data from the space radio telescope are corrected for a nonuniform reception band. We estimated the diameter of the scattering disk for this pulsar at a frequency of 1600 MHz: < 1.8 x 10^{-3} arcsec.

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