pith. sign in

arxiv: 1211.0753 · v1 · pith:C6JHEOM4new · submitted 2012-11-05 · 🌌 astro-ph.GA

Pilot Observations for MALT-45: A Galactic Plane Survey at 7mm

classification 🌌 astro-ph.GA
keywords surveydetectgalacticmalt-45pilotplanearoundarray
0
0 comments X p. Extension
pith:C6JHEOM4 Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{C6JHEOM4}

Prints a linked pith:C6JHEOM4 badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

We introduce the MALT-45 (Millimetre Astronomer's Legacy Team - 45 GHz) 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 of MALT-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 Broadband Backend (CABB) on the ATCA, we were able to observe two 2048 MHz spectral windows, centred on frequencies 43.2 and 48.2 GHz. Although only a coarse spectral resolution of around 7 km/s 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 1_1-0_0 A+ line.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.