TY - JOUR
T1 - Precision Southern Hemisphere pulsar vlbi astrometry
T2 - Techniques and results for PSR J1559-4438
AU - Deller, A. T.
AU - Tingay, S. J.
AU - Brisken, W.
PY - 2009
Y1 - 2009
N2 - We describe a data reduction pipeline for very long baseline interferometry astrometric observations of pulsars, implemented using the ParselTongue AIPS interface. The pipeline performs calibration (including ionosphere modeling), phase referencing with proper accounting for the reference source structure, amplitude corrections for pulsar scintillation, and position fitting to yield the position, proper motion, and parallax. The optimal data weighting scheme to minimize the total error budget of a parallax fit, and how this scheme varies with pulsar parameters such as flux density, is also investigated. The robustness of the techniques employed is demonstrated with the presentation of the first results from a two-year astrometry program using the Australian Long Baseline Array. The parallax of PSR J1559-4438 is determined to be 1π = 0.384 0.081 mas (1σ), resulting in a distance estimate of 2600 pc that is consistent with earlier dispersion measure and HI absorption stimates.
AB - We describe a data reduction pipeline for very long baseline interferometry astrometric observations of pulsars, implemented using the ParselTongue AIPS interface. The pipeline performs calibration (including ionosphere modeling), phase referencing with proper accounting for the reference source structure, amplitude corrections for pulsar scintillation, and position fitting to yield the position, proper motion, and parallax. The optimal data weighting scheme to minimize the total error budget of a parallax fit, and how this scheme varies with pulsar parameters such as flux density, is also investigated. The robustness of the techniques employed is demonstrated with the presentation of the first results from a two-year astrometry program using the Australian Long Baseline Array. The parallax of PSR J1559-4438 is determined to be 1π = 0.384 0.081 mas (1σ), resulting in a distance estimate of 2600 pc that is consistent with earlier dispersion measure and HI absorption stimates.
KW - Astrometry
KW - Pulsars: general
KW - Pulsars: individual (J1559?4438)
KW - Techniques: interferometric
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U2 - 10.1088/0004-637X/690/1/198
DO - 10.1088/0004-637X/690/1/198
M3 - Article
AN - SCOPUS:65549139476
SN - 0004-637X
VL - 690
SP - 198
EP - 209
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1
ER -