Research for Interstellar Scattering of Pulsar B0329+54 with VLBI

Details Research for Interstellar Scattering of Pulsar B0329+54 with VLBI Research for Interstellar Scattering of Pulsar B0329+54 with VLBI

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002evn..conf..251s&link_type=abstract

6th European VLBI Network Symposium on New Developments in VLBI Science and Technology, held in Bonn, June 25th-28th 2002, proce

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The talk deals with data reduction and result interpretation of SVLBI observations of pulsar B0329+54 at 1.6 GHz. The purpose of observations was scattering angle measurement. Additional steps for amplitude calibration of pulsar data (bandpass correction, correction for incommensurability of pulsar period and correlator integration time, correction for intrinsic pulsar variability) are invented. Software implementing these techniques was developed. Estimated size of scattering angle is less than 1.6 mas. An attempt to trace apparent source position changes induced by scattering has been made.

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