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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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