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<p style="mso-margin-top-alt:8.0pt;margin-right:0cm;margin-bottom:0cm;margin-left:0cm">
<span style="color:#1D1D1D">Dear All,</span><o:p></o:p></p>
<p style="mso-margin-top-alt:8.0pt;margin-right:0cm;margin-bottom:0cm;margin-left:0cm">
<span style="color:#1D1D1D"><o:p> </o:p></span></p>
<p style="mso-margin-top-alt:8.0pt;margin-right:0cm;margin-bottom:0cm;margin-left:0cm">
<span style="color:#1D1D1D">We are happy to announce the workshop for <b>DYNAMITE</b>, software for dynamical modelling of stellar systems, organised by ICRAR/UWA in collaboration with the “Stellar Dynamics” group at the University of Vienna. The workshop will
be held in <b>Perth, 5<sup>th</sup>-9<sup>th</sup> December 2022</b>. There is no registration fee to attend and a small amount of financial support for students for travel may be available. Further details can be found at the workshop website:</span><a href="https://protect-au.mimecast.com/s/V96hC81V0PTj5XAMxIntMSO?domain=icrar.org/"><span style="color:#1D1D1D">
</span><span style="color:#0A529F">DYNAMITE Workshop 2022</span></a><o:p></o:p></p>
<p style="mso-margin-top-alt:8.0pt;margin-right:0cm;margin-bottom:0cm;margin-left:0cm">
<span style="color:#1D1D1D">Registrations are now open (</span><a href="https://protect-au.mimecast.com/s/O0Y4C91WPRTmWz6KPCEeqm2?domain=icrar.org/"><span style="color:#0A529F">Registration</span></a><span style="color:#1D1D1D">). Please register your attendance
by <b>Friday 28<sup>th</sup> October</b>. </span><o:p></o:p></p>
<p style="mso-margin-top-alt:8.0pt;margin-right:0cm;margin-bottom:0cm;margin-left:0cm">
<span style="color:#1D1D1D">The workshop will be aimed at making dynamical modelling more accessible to the broader astronomical community. Face-to-face attendance is encouraged, but we will provide remote access to interested people. </span><o:p></o:p></p>
<p style="mso-margin-top-alt:8.0pt;margin-right:0cm;margin-bottom:0cm;margin-left:0cm">
<span style="color:#1D1D1D">Schwarzschild dynamical models, while successfully used for numerous scientific projects over the last 15 years, were only recently used to model a large number of galaxies (first used for ~300 galaxies from the CALIFA survey, ~150
from the MaNGA survey and ~160 from the SAMI surveys). With new data coming from state-of-the-art IFS surveys such as MAGPI and HECTOR, being able to exploit all the information we can derive from good quality data is crucial. DYNAMITE (DYnamics, Age and Metallicity
Indicators Tracing Evolution) is a next generation implementation of the Schwarzschild technique for orbit-based dynamical modelling of stellar systems. DYNAMITE’s great versatility makes it the perfect tool for a vast variety of projects and astronomical
fields. This workshop will provide the tools to enable scientists to use such a powerful technique in their research, maximising their research outputs.</span><o:p></o:p></p>
<p style="mso-margin-top-alt:8.0pt;margin-right:0cm;margin-bottom:0cm;margin-left:0cm">
<span style="color:#1D1D1D">If you have any questions, please contact me (<a href="mailto:giulia.santucci@uwa.edu.au">giulia.santucci@uwa.edu.au</a>).<o:p></o:p></span></p>
<p style="mso-margin-top-alt:8.0pt;margin-right:0cm;margin-bottom:0cm;margin-left:0cm">
<span style="color:#1D1D1D">We look forward to you joining us in Perth!</span><o:p></o:p></p>
<p class="MsoNormal"><span style="font-size:11.0pt"><o:p> </o:p></span></p>
<p class="MsoNormal"><span style="font-size:11.0pt">Best regards,<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-size:11.0pt">Giulia<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-size:11.0pt"><o:p> </o:p></span></p>
<p class="MsoNormal"><span style="font-size:11.0pt"><o:p> </o:p></span></p>
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<p class="MsoNormal" style="background:white;vertical-align:baseline"><span style="color:black;border:none windowtext 1.0pt;padding:0cm;mso-fareast-language:EN-GB">----------------------------------</span><span style="font-size:11.0pt;color:black;mso-fareast-language:EN-GB"><o:p></o:p></span></p>
<p class="MsoNormal" style="background:white;vertical-align:baseline"><span style="color:black;border:none windowtext 1.0pt;padding:0cm;mso-fareast-language:EN-GB">Dr Giulia Santucci (she/her)</span><span style="font-size:11.0pt;color:black;mso-fareast-language:EN-GB"><o:p></o:p></span></p>
<p class="MsoNormal" style="background:white;vertical-align:baseline"><span style="color:black;border:none windowtext 1.0pt;padding:0cm;mso-fareast-language:EN-GB">Postdoctoral Research Associate</span><span style="font-size:11.0pt;color:black;mso-fareast-language:EN-GB"><o:p></o:p></span></p>
<p class="MsoNormal" style="background:white;vertical-align:baseline"><span style="color:black;border:none windowtext 1.0pt;padding:0cm;mso-fareast-language:EN-GB">International Centre for Radio Astronomy Research (ICRAR)</span><span style="font-size:11.0pt;color:black;mso-fareast-language:EN-GB"><o:p></o:p></span></p>
<p class="MsoNormal" style="background:white;vertical-align:baseline"><span style="color:black;border:none windowtext 1.0pt;padding:0cm;mso-fareast-language:EN-GB">University of Western Australia</span><span style="font-size:11.0pt;color:black;mso-fareast-language:EN-GB"><o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-size:10.0pt;color:black;mso-fareast-language:EN-GB">I sent this email at a time that is convenient for me. I do not expect a response outside of your normal working hours.</span><span style="font-size:11.0pt;color:black;mso-fareast-language:EN-GB"><o:p></o:p></span></p>
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