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<p class="MsoNormal"><span style="color:#212121">Dear colleagues, </span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121"> </span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">We are pleased to announce that registration is now open for the meeting “Galaxy Transformation Across Space and Time” to be held in Canberra this coming September. Please visit<span class="apple-converted-space"> </span><a href="https://protect-au.mimecast.com/s/u6SFC1WLPxc6Kyo8GIL9oO1?domain=mso.anu.edu.au/" title="Original URL:
https://www.mso.anu.edu.au/~jtmendel/galtrans2023/
Click to follow link."><span style="color:#0078D7">https://www.mso.anu.edu.au/~jtmendel/galtrans2023/</span></a><span class="apple-converted-space"> </span>for
more information.</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121"> </span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">A preliminary schedule for the meeting is available on the conference website. Although talk abstract submissions are now closed, we are still accepting poster abstracts via this link:<span class="apple-converted-space"> </span><a href="https://protect-au.mimecast.com/s/LcGbC2xMQziVAqX73f1f-nx?domain=forms.gle" title="Original URL:
https://forms.gle/JZnU14yqgGYdq26y7
Click to follow link."><span style="color:#0078D7">https://forms.gle/JZnU14yqgGYdq26y7</span></a><o:p></o:p></span></p>
<p class="MsoNormal"><span style="color:#212121"><o:p> </o:p></span></p>
<p class="MsoNormal"><span style="color:#212121">We hope to see you in Canberra in September!</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<b><span style="color:#212121"> </span></b><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<b><span style="color:#212121"> </span></b><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<b><span style="color:#212121">Galaxy Transformation Across Space and Time</span></b><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">--- The 3rd Australia-ESO meeting ---</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">4-8 September 2023</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Australian Academy of Science, Canberra, Australia</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121"><a href="https://protect-au.mimecast.com/s/u6SFC1WLPxc6Kyo8GIL9oO1?domain=mso.anu.edu.au/" title="Original URL:
https://www.mso.anu.edu.au/~jtmendel/galtrans2023/
Click to follow link."><span style="color:#0078D7">https://www.mso.anu.edu.au/~jtmendel/galtrans2023/</span></a></span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121"> </span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<b><span style="color:#212121">Rational / Key Questions:<span class="apple-converted-space"> </span></span></b><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Galaxies transform throughout their lifetimes as a result of internal processes, interactions with other galaxies, their environments, and the cosmic web. The interplay of these processes alters the distribution of properties used
to characterise the galaxy population. Understanding the impact and relative importance of that interplay is critical to galaxy evolution as whole. With new capabilities enabling highly-resolved investigations of gas and stars in local galaxies, it is now
possible to disentangle detailed star-formation and assembly histories for a wide variety of galaxy types. Simultaneously, surveys pushing resolved observations to earlier epochs are providing important constraints on the evolution and transformation of dynamics
and chemical distributions. Together these approaches have the power to discern complex assembly histories over the last 7-10 Gyrs, when simulations suggest that dramatic morphological and kinematic evolution is expected to occur. However, the exact timing
and nature of these transformations are debated.<span class="apple-converted-space"> </span></span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121"> </span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">In this conference we aim to connect observations and simulations of galaxy transformations across cosmic time, with a particular focus on the following questions:</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121"> </span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">• How does environment shape the star-formation history of galaxies?</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">• How do we connect galaxy populations across epochs?</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">• What is the environmental impact on redistributing angular momentum?</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">• How do stellar and AGN feedback regulate the gas-star formation cycle at z~0?</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121"> </span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<b><span style="color:#212121">Confirmed Invited Speakers:</span></b><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Caroline Bertemes (ARI)</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Deanne Fisher (Swinburne)</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Joel Leja (Penn State)</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Danail Obreschkow (ICRAR/UWA)</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Benedetta Vulcani (INAF)</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Charlotte Welker (Johns Hopkins)</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121"> </span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<b><span style="color:#212121">SOC:</span></b><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Trevor Mendel (co-chair)</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Emily Wisnioski (co-chair)</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Barbara Catinella</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Michelle Cluver</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Mirko Curti</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Harald Kuntschner</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Rhea Silvia Remus</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Jesse van de Sande</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Edward Taylor</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Ling Zhu</span><span style="font-size:10.0pt;color:#212121"><o:p></o:p></span></p>
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