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<p class="MsoNormal"><span style="color:#212121">Dear colleagues, <o:p></o:p></span></p>
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<span style="color:#212121"> <o:p></o:p></span></p>
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<span style="color:#212121">We are extended abstract submission for the meeting “Galaxy Transformation Across Space and Time” to be held in Canberra this coming September. The new deadline is
<b>Monday, May 8<sup>th</sup></b>. Please circulate this announcement amongst your networks.<o:p></o:p></span></p>
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<b><span style="color:#212121"> </span></b><span style="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="color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">--- The 3rd Australia-ESO meeting ---<o:p></o:p></span></p>
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<span style="color:#212121">4-8 September 2023<o:p></o:p></span></p>
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<span style="color:#212121">Australian Academy of Science, Canberra, Australia<o:p></o:p></span></p>
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<span style="color:#212121"><a href="https://protect-au.mimecast.com/s/oVsRCZY1Nqi7QKMMwszyOdI?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><o:p></o:p></span></p>
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<span style="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="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><o:p></o:p></span></p>
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<span style="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:<o:p></o:p></span></p>
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<span style="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?<o:p></o:p></span></p>
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<span style="color:#212121">• How do we connect galaxy populations across epochs?<o:p></o:p></span></p>
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<span style="color:#212121">• What is the environmental impact on redistributing angular momentum?<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?<o:p></o:p></span></p>
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<span style="color:#212121"> <o:p></o:p></span></p>
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<b><span style="color:#212121">Confirmed Invited Speakers:</span></b><span style="color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Caroline Bertemes (ARI)<o:p></o:p></span></p>
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<span style="color:#212121">Deanne Fisher (Swinburne)<o:p></o:p></span></p>
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<span style="color:#212121">Joel Leja (Penn State)<o:p></o:p></span></p>
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<span style="color:#212121">Danail Obreschkow (ICRAR/UWA)<o:p></o:p></span></p>
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<span style="color:#212121">Benedetta Vulcani (INAF)<o:p></o:p></span></p>
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<span style="color:#212121">Charlotte Welker (Johns Hopkins)<o:p></o:p></span></p>
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<span style="color:#212121"> <o:p></o:p></span></p>
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<b><span style="color:#212121">Important dates:</span></b><span style="color:#212121"><o:p></o:p></span></p>
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<i><span style="color:#212121">Abstract submission deadline:</span></i><span style="color:#212121">
<b>8 May 2023</b><o:p></o:p></span></p>
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<i><span style="color:#212121">Program announcement, registration opens:</span></i><span style="color:#212121"> 1 June 2023<o:p></o:p></span></p>
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<i><span style="color:#212121">Meeting:</span></i><span class="apple-converted-space"><span style="color:#212121"> </span></span><span style="color:#212121"> 4-8 September 2023<o:p></o:p></span></p>
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<span style="color:#212121"> <o:p></o:p></span></p>
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<b><span style="color:#212121">Abstract submission:<span class="apple-converted-space"> </span></span></b><span style="color:#212121"><a href="https://protect-au.mimecast.com/s/L-rEC1WLPxc6qJpp0TG9yno?domain=forms.gle" title="https://aus01.safelinks.protection.outlook.com/?url=https%3A%2F%2Fforms.gle%2FJZnU14yqgGYdq26y7&data=05%7C01%7Ctrevor.mendel%40anu.edu.au%7C3a4095cfd04b4957d3da08db41911640%7Ce37d725cab5c46249ae5f0533e486437%7C0%7C0%7C638175863626018030%7CUnknown%7CTWFpbG"><span style="color:#0078D7">https://forms.gle/JZnU14yqgGYdq26y7</span></a><o:p></o:p></span></p>
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<span style="color:#212121"> <o:p></o:p></span></p>
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<b><span style="color:#212121">SOC:</span></b><span style="color:#212121"><o:p></o:p></span></p>
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<span style="color:#212121">Trevor Mendel (co-chair)<o:p></o:p></span></p>
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<span style="color:#212121">Emily Wisnioski (co-chair)<o:p></o:p></span></p>
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<span style="color:#212121">Barbara Catinella<o:p></o:p></span></p>
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<span style="color:#212121">Michelle Cluver<o:p></o:p></span></p>
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<span style="color:#212121">Mirko Curti<o:p></o:p></span></p>
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<span style="color:#212121">Harald Kuntschner<o:p></o:p></span></p>
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<span style="color:#212121">Rhea Silvia Remus<o:p></o:p></span></p>
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<span style="color:#212121">Jesse van de Sande<o:p></o:p></span></p>
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<span style="color:#212121">Edward Taylor<o:p></o:p></span></p>
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<span style="color:#212121">Ling Zhu<o:p></o:p></span></p>
<p class="MsoNormal"><o:p> </o:p></p>
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