Data

LBA observations for project V645 semester 2024APRS

Commonwealth Scientific and Industrial Research Organisation
Phillips, Chris ; Ekers, Ron ; Garrett, Mike ; Reynolds, Cormac ; Price, Danny
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=https://data.csiro.au/collection/csiro:CASDA-ATOA-V645-2024APRS?tab=data DataDownload&rft.title=LBA observations for project V645 semester 2024APRS&rft.identifier=http://hdl.handle.net/102.100.100/705923?index=1&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=Traditionally searches for techno-signatures have utilised raw voltage data from single-dish radio telescopes or beam-formed data from radio arrays with relatively short baselines. We propose a short LBA observation as a pilot experiment to explore the options for utilising VLBI for SETI searches. Widely separated telescopes are naturally more immune to confusion from RFI sources, and the phase response from any detection can be used to distinguish terrestrial signals from distant emitters (past the moon).&rft.creator=Phillips, Chris &rft.creator=Ekers, Ron &rft.creator=Garrett, Mike &rft.creator=Reynolds, Cormac &rft.creator=Price, Danny &rft.date=2025&rft.edition=v1&rft_rights=Creative Commons Attribution 4.0 International Licence https://creativecommons.org/licenses/by/4.0/&rft_rights=Data is accessible online and may be reused in accordance with licence conditions&rft_rights=All Rights (including copyright) CSIRO 2025.&rft_subject=exoplanets&rft_subject=Astronomical sciences not elsewhere classified&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft.type=dataset&rft.language=English Access the data
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Traditionally searches for techno-signatures have utilised raw voltage data from single-dish radio telescopes or beam-formed data from radio arrays with relatively short baselines. We propose a short LBA observation as a pilot experiment to explore the options for utilising VLBI for SETI searches. Widely separated telescopes are naturally more immune to confusion from RFI sources, and the phase response from any detection can be used to distinguish terrestrial signals from distant emitters (past the moon).

Available: 2025-05-09

Data time period: 2024-04-01 to 2024-09-30

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Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | Physical Sciences | exoplanets |

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