Pilot observations for MALT-45: a Galactic plane survey at 7 mm

We introduce the Millimetre Astronomer’s Legacy Team – 45 GHz (MALT-45) Galactic plane survey and describe pilot survey results with the Australia Telescope Compact Array (ATCA).The pilot survey was conducted to test the instrumentation and observational technique ofMALT-45, before commencing the fu...

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Main Authors: Jordan, C., Walsh, Andrew, Lowe, V., Lo, N., Purcell, C., Voronkov, M., Longmore, S.
Format: Journal Article
Published: Oxford University Press 2013
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/4770
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author Jordan, C.
Walsh, Andrew
Lowe, V.
Lo, N.
Purcell, C.
Voronkov, M.
Longmore, S.
author_facet Jordan, C.
Walsh, Andrew
Lowe, V.
Lo, N.
Purcell, C.
Voronkov, M.
Longmore, S.
author_sort Jordan, C.
building Curtin Institutional Repository
collection Online Access
description We introduce the Millimetre Astronomer’s Legacy Team – 45 GHz (MALT-45) Galactic plane survey and describe pilot survey results with the Australia Telescope Compact Array (ATCA).The pilot survey was conducted to test the instrumentation and observational technique ofMALT-45, before commencing the full survey. We mapped two half-square degree regions within the southern Galactic plane around the G333 giant molecular cloud, using fast mosaic mapping. Using the new Compact Array Broad-band Backend on the ATCA, we were able to observe two 2048MHzspectral windows, centred on frequencies 43.2 and 48.2 GHz. Although only a coarse spectral resolution of around 7 km s-1 was available to us, we detect widespread, extended emission in the CS (1–0) ground state transition. We also detect eight Class I CH3OH masers at 44 GHz and three SiO masers in vibrationally excited (1–0) transitions. We also detect the H53a radio recombination line, non-vibrationally excited SiO (1–0) and emission in the CH3OH 11–00 A+ line.
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institution Curtin University Malaysia
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publishDate 2013
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spelling curtin-20.500.11937-47702017-09-13T14:45:09Z Pilot observations for MALT-45: a Galactic plane survey at 7 mm Jordan, C. Walsh, Andrew Lowe, V. Lo, N. Purcell, C. Voronkov, M. Longmore, S. structure radio - lines stars Galaxy masers molecules surveys ISM formation We introduce the Millimetre Astronomer’s Legacy Team – 45 GHz (MALT-45) Galactic plane survey and describe pilot survey results with the Australia Telescope Compact Array (ATCA).The pilot survey was conducted to test the instrumentation and observational technique ofMALT-45, before commencing the full survey. We mapped two half-square degree regions within the southern Galactic plane around the G333 giant molecular cloud, using fast mosaic mapping. Using the new Compact Array Broad-band Backend on the ATCA, we were able to observe two 2048MHzspectral windows, centred on frequencies 43.2 and 48.2 GHz. Although only a coarse spectral resolution of around 7 km s-1 was available to us, we detect widespread, extended emission in the CS (1–0) ground state transition. We also detect eight Class I CH3OH masers at 44 GHz and three SiO masers in vibrationally excited (1–0) transitions. We also detect the H53a radio recombination line, non-vibrationally excited SiO (1–0) and emission in the CH3OH 11–00 A+ line. 2013 Journal Article http://hdl.handle.net/20.500.11937/4770 10.1093/mnras/sts350 Oxford University Press fulltext
spellingShingle structure
radio - lines
stars
Galaxy
masers
molecules
surveys
ISM
formation
Jordan, C.
Walsh, Andrew
Lowe, V.
Lo, N.
Purcell, C.
Voronkov, M.
Longmore, S.
Pilot observations for MALT-45: a Galactic plane survey at 7 mm
title Pilot observations for MALT-45: a Galactic plane survey at 7 mm
title_full Pilot observations for MALT-45: a Galactic plane survey at 7 mm
title_fullStr Pilot observations for MALT-45: a Galactic plane survey at 7 mm
title_full_unstemmed Pilot observations for MALT-45: a Galactic plane survey at 7 mm
title_short Pilot observations for MALT-45: a Galactic plane survey at 7 mm
title_sort pilot observations for malt-45: a galactic plane survey at 7 mm
topic structure
radio - lines
stars
Galaxy
masers
molecules
surveys
ISM
formation
url http://hdl.handle.net/20.500.11937/4770