Characterisation of the MALT90 survey and the Mopra telescope at 90 GHz

Characterisation of the MALT90 survey and the Mopra telescope at 90 GHz

We characterise the Millimetre Astronomy Legacy Team 90 GHz Survey (MALT90) and the Mopra telescope at 90 GHz. We combine repeated position-switched observations of the source G300.968+01.145 with a map of the same source in order to estimate the pointing reliability of the position-switched observa...

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Bibliographic Details
Main Authors: Walsh, Andrew, Foster, J. B., Rathborne, J. M., Sanhueza, P., Claysmith, C., Whitaker, J. S., Jackson, J. M., Mascoop, J. L., Wienen, M., Breen, S. L., Herpin, F., Duarte-Cabral, A., Csengeri, T., Contreras, Y., Indermuehle, B., Barnes, P. J., Cunningham, M. R., Britton, T. R., Voronkov, M. A., Urquhart, J. S., Alves, J., Jordan, C. H., Hill, T., Hoq, S., Brooks, K. J., Longmore, S. N.
Format: Journal Article
Published: CSIRO 2013
Subjects:
instrumentation: spectrographs
ISM: individual (RCW 65)
telescopes
radio lines: ISM
H II regions
astrochemistry
Online Access:http://hdl.handle.net/20.500.11937/18209

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