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Magellanic clouds and nearby galaxies
Magellanic clouds and nearby galaxies
Team lead: Dr Ivy Wong
Members: Bi-Qing For, Bryan Gaensler, Tim Galvin, George Heald, Natasha Hurley-Walker, Philippa Patterson, Maria Rioja, Lister Staveley-Smith, Hongquan Su, Tsutomu Takeuchi, Jennifer West, Ivy Wong, + (please add your name if you're interested in joining the team)
Recent submissions:
- Submitted to ApJ by Anna Kapińska et al 2019 "Physical processes and detectability of star-forming Sculptor Group galaxies at low radio frequencies"
Recent publications:
- Published MNRAS paper by Bi-Qing For et al 2018 "A Multi-Frequency Radio Continuum Study of the Magellanic Clouds. I. Overall Structure and Star Formation Rates
- Link to ADS: http://adsabs.harvard.edu/abs/2018MNRAS.480.2743F
- Published ApJ paper by Anna Kapińska et al 2017 "Spectral Energy Distribution and Radio Halo of NGC 253 at Low Radio Frequencies
- Link to ADS: http://adsabs.harvard.edu/abs/2017ApJ...838...68K
Projects in progress:
- MWA Phase 2 observations of LMC+SMC (Patterson, Staveley-Smith et al): work by Masters student Philippa Patterson
- thesis completed December 2020; however not all data reduction is complete for the LMC so please speak to Lister if interested)
- MWA Phase 2 observations of M83 (Tim Galvin et al)
- MWA (Phase 1 /Gleam) + Spitzer observations of NGC 7793 (Navabi, Wong et al ): work by "summer student" at UWA aimed at investigating the resolved radio-FIR properties of NGC 7793 – project ended
- MWA(Phase 1) + multiwavelength observations of Virgo Cluster Galaxies (Yoshida, S, Takeuchi, T. et al): work by Masters student at Nagoya under the supervision of Tsutomu with minor supervision by Luca Cortese, Barbara Catinella & Ivy Wong (esp. for a winter studentship at ICRAR/UWA)
- Shuntaro Yoshida has finished his studies and left the project but Tsutomu & his Nagoya team will take over the project to finish it.
- Low-frequency SED of Swift BAT Hard X-ray-selected nearby galaxies (Wong, Kapińska et al ) : Phase 1 data had insufficient angular resolution and now awaiting Phase 2 data
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