The Transient Array Radio Telescope: An open-source all-sky imaging radio interferometer

The Transient Array Radio Telescope (TART) is an open-source 24-element 1573-1577 MHz L-band imaging interferometer designed for research and education. This paper introduces the physical architecture of the TART, describes it's electronics, radios, correlator, and the design of the antenna array. Then we discuss the software architecture, including the calibration of the telescope using satellites and imaging pipelines. Imaging results are presented, which lead to an estimate of ~52 kJy for the sensitivity of the telescope.

Authors

Publication Details

Journal
arXiv (Cornell University)
Published
2026-11-02
DOI
https://doi.org/10.48550/arxiv.2611.02313
Primary Topic
Radio Astronomy Observations and Technology
Type
preprint
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preprint

The Transient Array Radio Telescope: An open-source all-sky imaging radio interferometer

Max Scheel, Pat Suggate, T. C. A. Molteno, Phil Brown et al.
arXiv (Cornell University)
Radio Astronomy Observations and Technology
preprint

The Transient Array Radio Telescope: An open-source all-sky imaging radio interferometer

Max Scheel, Pat Suggate, T. C. A. Molteno, Phil Brown, Ben V. Hugo
preprint en

Abstract

The Transient Array Radio Telescope (TART) is an open-source 24-element 1573-1577 MHz L-band imaging interferometer designed for research and education. This paper introduces the physical architecture of the TART, describes it's electronics, radios, correlator, and the design of the antenna array. Then we discuss the software architecture, including the calibration of the telescope using satellites and imaging pipelines. Imaging results are presented, which lead to an estimate of ~52 kJy for the sensitivity of the telescope.

arXiv (Cornell University)
Radio Astronomy Observations and Technology
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