Data

The Mopra SiO Maser Catalogue

Commonwealth Scientific and Industrial Research Organisation
Indermuehle, Balthasar ; Edwards, Phil ; Brooks, Kate ; Urquhart, James
Viewed: [[ro.stat.viewed]] Cited: [[ro.stat.cited]] Accessed: [[ro.stat.accessed]]
ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.4225/08/521A8EF38E042&rft.title=The Mopra SiO Maser Catalogue&rft.identifier=https://doi.org/10.4225/08/521A8EF38E042&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=The Mopra project M426 was started in 2008 to regularly monitor all bright SiO masers visible from the Mopra radio telescope near the township of Coonabarabran in northwestern New South Wales. A total of 121 SiO masers, thereof 47 LPVs, have been observed between April 2008 and August 2013 in both v=1, J=1-0 (43.122 GHz) and the v=1, J=2-1 (86.2434 GHz) transitions. Each source has been observed between 25 and 50 times during that time span.Lineage: The data has been obtained using the Mopra radio telescope and the UNSW-MOPS digital spectrometer.&rft.creator=Indermuehle, Balthasar &rft.creator=Edwards, Phil &rft.creator=Brooks, Kate &rft.creator=Urquhart, James &rft.date=2013&rft.edition=v1&rft_rights=CSIRO Data Licence https://research.csiro.au/dap/licences/csiro-data-licence/&rft_rights=Data is accessible online and may be reused in accordance with licence conditions&rft_rights=All Rights (including copyright) CSIRO Australia 2013.&rft_subject=astronomical masers&rft_subject=Stellar astronomy and planetary systems&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft.type=dataset&rft.language=English Access the data
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The Mopra project M426 was started in 2008 to regularly monitor all bright SiO masers visible from the Mopra radio telescope near the township of Coonabarabran in northwestern New South Wales. A total of 121 SiO masers, thereof 47 LPVs, have been observed between April 2008 and August 2013 in both v=1, J=1-0 (43.122 GHz) and the v=1, J=2-1 (86.2434 GHz) transitions. Each source has been observed between 25 and 50 times during that time span.
Lineage: The data has been obtained using the Mopra radio telescope and the UNSW-MOPS digital spectrometer.

Available: 2013-08-26

Data time period: 2008-04-01 to 2013-08-23

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Subjects
Astronomical Sciences | Physical Sciences | Stellar Astronomy and Planetary Systems | astronomical masers |

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Identifiers
ACN 633 798 857