GASV: A New VLBI analysis software for Geodesy and Astrometry

Fuente: arXiv
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Autori principali: Yao, Dang, Wu, Yuan-wei, Yang, Xu-hai
Natura: Preprint
Pubblicazione: 2026
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author Yao, Dang
Wu, Yuan-wei
Yang, Xu-hai
author_facet Yao, Dang
Wu, Yuan-wei
Yang, Xu-hai
contents We present GASV, a novel Python-based software package specifically designed for the analysis of Very Long Baseline Interferometry (VLBI) data. Developed with ease of installation and user friendliness in mind, GASV supports both pipeline and interactive processing modes. The software processes VLBI baseline delays and rates in standard formats such as HOPS outputs and NGS card files to estimate key geodetic and astrometric parameters, including station coordinates, Earth Orientation Parameters, source coordinates, clock parameters, and atmospheric models. We evaluate the capabilities and performance of GASV, demonstrating that its parameter estimation accuracy for IVS INT, Regular, and CONT sessions is comparable to that achieved by the VLBI analysis centers at BKG and USNO. As a state-of-the-art tool, GASV not only enables high-quality single-session data processing but also but also supports global analyses of long-term SINEX files, generating Celestial Reference Frame and Terrestrial Reference Frame solutions with reliable accuracy.
format Preprint
id arxiv_https___arxiv_org_abs_2602_04183
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle GASV: A New VLBI analysis software for Geodesy and Astrometry
Yao, Dang
Wu, Yuan-wei
Yang, Xu-hai
Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
85A02
J.2.3
We present GASV, a novel Python-based software package specifically designed for the analysis of Very Long Baseline Interferometry (VLBI) data. Developed with ease of installation and user friendliness in mind, GASV supports both pipeline and interactive processing modes. The software processes VLBI baseline delays and rates in standard formats such as HOPS outputs and NGS card files to estimate key geodetic and astrometric parameters, including station coordinates, Earth Orientation Parameters, source coordinates, clock parameters, and atmospheric models. We evaluate the capabilities and performance of GASV, demonstrating that its parameter estimation accuracy for IVS INT, Regular, and CONT sessions is comparable to that achieved by the VLBI analysis centers at BKG and USNO. As a state-of-the-art tool, GASV not only enables high-quality single-session data processing but also but also supports global analyses of long-term SINEX files, generating Celestial Reference Frame and Terrestrial Reference Frame solutions with reliable accuracy.
title GASV: A New VLBI analysis software for Geodesy and Astrometry
topic Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
85A02
J.2.3
url https://arxiv.org/abs/2602.04183