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dc.contributorSchool of Physics, University of New South Wales, Sydney, NSW 2052, Australia
dc.contributorSchool of Physics, University of New South Wales, Sydney, NSW 2052, Australia; School of Computing Engineering and Mathematics, Western Sydney University, Locked Bay 1797, Penrith, NSW 2751, Australia
dc.contributorSchool of Physics, University of New South Wales, Sydney, NSW 2052, Australia; Armagh Observatory and Planetarium, College Hill, Armagh BT61 9DG, UK
dc.contributorSchool of Physical Sciences, University of Adelaide, Adelaide, SA 5005, Australia
dc.contributorSchool of Computing Engineering and Mathematics, Western Sydney University, Locked Bay 1797, Penrith, NSW 2751, Australia
dc.contributorCSIRO Astronomy & Space Science, Australia Telescope National Facility, PO Box 76, Epping, NSW 2121, Australia
dc.contributorJoint ALMA Observatory, Alonso de Córdova 3107, Vitacura, Santiago, Chile; National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USA
dc.contributor.authorBraiding, Catherine
dc.contributor.authorWong, G. F.
dc.contributor.authorMaxted, N. I.
dc.contributor.authorRomano, D.
dc.contributor.authorBurton, M. G.
dc.contributor.authorBlackwell, R.
dc.contributor.authorFilipović, M. D.
dc.contributor.authorFreeman, M. S. R.
dc.contributor.authorIndermuehle, B.
dc.contributor.authorLau, J.
dc.contributor.authorRebolledo, D.
dc.contributor.authorRowell, G.
dc.contributor.authorSnoswell, C.
dc.contributor.authorTothill, N. F. H.
dc.contributor.authorVoisin, F.
dc.contributor.authorde Wilt, P.
dc.date.accessioned2024-02-21T11:02:40Z
dc.date.available2024-02-21T11:02:40Z
dc.date.issued2018-08-01T00:00:00Z
dc.identifier.doi10.1017/pasa.2018.18
dc.identifier.doi10.48550/arXiv.1902.04249
dc.identifier.other2018PASA...35.e029B
dc.identifier.other2019arXiv190204249B
dc.identifier.otherastro-ph.GA
dc.identifier.other2018PASA...35...29B
dc.identifier.other10.1017/pasa.2018.18
dc.identifier.otherarXiv:1902.04249
dc.identifier.other10.48550/arXiv.1902.04249
dc.identifier.other2019arXiv190204249B
dc.identifier.other2018PASA...35.e029B
dc.identifier.other-
dc.identifier.other0000-0003-1479-7949
dc.identifier.urihttp://hdl.handle.net/20.500.14302/1648
dc.description.abstractWe present observations of 50 deg<SUP>2</SUP> of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes l = 300-350° and latitudes |b| ⩽ 0.5°. These data have been taken at 0.6 arcmin spatial resolution and 0.1 km s<SUP>-1</SUP>spectral resolution, providing an unprecedented view of the molecular clouds and gas of the Southern Galactic Plane in the 109-115 GHz J = 1-0 transitions of <SUP>12</SUP>CO, <SUP>13</SUP>CO, C<SUP>18</SUP>O, and C<SUP>17</SUP>O.
dc.publisherPublications of the Astronomical Society of Australia
dc.titleThe Mopra Southern Galactic Plane CO Survey—Data Release 3
dc.typearticle
dc.source.journalPASA
dc.source.journalPASA...35
dc.source.volume35
refterms.dateFOA2024-02-21T11:02:40Z
dc.identifier.bibcode2018PASA...35...29B


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