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DTSTART;TZID=Australia/Sydney:20251121T080000
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DTSTAMP:20260515T163310
CREATED:20251203T010158Z
LAST-MODIFIED:20251203T010415Z
UID:16319-1763712000-1765904400@www.atnf.csiro.au
SUMMARY:Apply for the 2026APR semester
DESCRIPTION:Overview\n\nWe’re pleased to announce that proposals for ATNF observing time are now open for the 2026APR semester. Grab your chance to use some of our new receivers and facilities. \n\nApply now for: \n\n\nOur ASKAP radio telescope (including CRACO)\n\n\n\nOur Australia Telescope Compact Array\n\n\n\nMurriyang\, our 64-m Parkes radio telescope\n\n\n\nThe Tidbinbilla radio antennas: the 70-m antenna Ballima (DSS-43) \, and the 34-m (DSS-34) antenna;\n\n\n\nThe Long Baseline Array\n\n\nMark your calendars: the deadline for all proposals is 06:00 UT (17:00 Sydney local time) on Tuesday\, 16 December 2025. \n\nTo submit your proposal\, visit our online proposal application system\, OPAL. \nMore information\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColloquia
URL:https://www.atnf.csiro.au/event/apply-for-the-2026apr-semester/
LOCATION:NSW
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/09/E9A915740-OBERSVERS-6-scaled.jpg
ORGANIZER;CN="George Hobbs":MAILTO:george.hobbs@csiro.au
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DTSTART;TZID=Australia/Sydney:20251203T120000
DTEND;TZID=Australia/Sydney:20251203T130000
DTSTAMP:20260515T163310
CREATED:20251118T071516Z
LAST-MODIFIED:20251127T060200Z
UID:16181-1764763200-1764766800@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Sam Taziaux (Ruhr University Bochum)
DESCRIPTION:MEDUSA  — Magnetic-field Evolution in Dwarf galaxies from Ultra-deep SKA Analysis  \n\n\nAbstract: \n\nDwarf galaxies are an important class of galaxies\, which are known to serve as proxy for the early Universe and play a crucial role in the formation and evolution of larger galaxies. To understand the underlying emission mechanism and the physics that drive the radiation far away from their origin\, we perform radio continuum polarimetry studies using deep MeerKAT observations. With the MEDUSA (Magnetic field Evolution in Dwarf galaxies Using SKA Analysis) project\, we present to-date the largest radio polarimetry study of dwarf galaxies\, including HI kinematics. Analysis of the spectrum reveals potential energy losses with rapid dissipation of electrons over kiloparsec scales\, a phenomenon contrasting sharply with observations from grand spiral galaxies. Furthermore\, small-scale dynamos in the star-fomation knots and a correlation between the level of depolarisation and the star formation histories deepen the understanding of this low mass systems. These findings provide evidence of intense material feedback into the intergalactic medium\, a process expected to be prevalent in the protogalaxies of the early Universe.  \n\nPlease note that the event timezone is AWST (UTC+8 hrs) \nJoin Event on Microsoft Teams\nLocation\n\nOrganiser\n\n \n\n \n\nEvent details\nDownload iCal\nCategory\nColloquia
URL:https://www.atnf.csiro.au/event/sa-colloquium-sam-taziaux-ruhr-university-bochum/
LOCATION:26 Dick Perry Ave\, Kensington WA 6151\, 26 Dick Perry Avenue\, Kensington\, Washington\, 6151
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/png:https://www.atnf.csiro.au/wp-content/uploads/2025/11/sam_taziaux_apad.png
ORGANIZER;CN="Gemma Anderson":MAILTO:gemma.anderson@csiro.au
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