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- PI: James Allison
- Frequency: Centred at 215MHz
Molecular Transitions in Vela and Orion (G0018)
- PI: Chenoa Tremblay
- Frequency: 99–129MHz
Molecular Lines in the Galactic Centre (G0018)
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- PI: Christoph Weniger (MWA members Ramesh Bhat and Chenoa Tremblay)
- Frequency: 70-300MHz
Paper Proposals:
Tremblay, Chenoa et al. "Continuum Survey of HII region in the Vela Constellation with MWA and ASKAP"
Publications:
Tremblay, Chenoa et al. "Nitric Oxide and other molecules: Molecular Modelling and Low Frequency Exploration using the Murchison Widefield Array"
Tremblay, Chenoa et al. "Continuum Survey of HII region in the Vela Constellation with MWA and ASKAP"
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(https://ui.adsabs.harvard.edu/abs/2020arXiv201009868T/abstract)
Tremblay, C.D. , Tingay, S.J. "A SETI Survey of the Vela Region using the Murchison Widefield Array: Orders of Magnitude Expansion in Search Space" Submitted to PASAPASA 2020PASA...37...35T (https://ui.adsabs.harvard.edu/abs/2020PASA...37...35T/abstract)
Tremblay, Chenoa "A Search for Molecules at Low Frequency with the Murchison Widefield Array" Ph.D. Thesis (https://ui.adsabs.harvard.edu/#abs/2018PhDT........52T/abstract)
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