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<b class=""><span class="" style="font-size:22pt; font-family:"Helvetica Neue"">Final Announcement </span></b></div>
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<a href="https://protect-au.mimecast.com/s/J3lhCK1DvKT2yOG4KhMSBP-?domain=indico.ict.inaf.it/" title="https://indico.ict.inaf.it/event/1547/" class=""><b class=""><span class="" style="font-size:22pt; font-family:"Helvetica Neue"; color:rgb(70,135,255)">HRMOS Science Workshop</span></b><b class=""><span class="" style="font-size:22pt; font-family:"Helvetica Neue"; color:black"> </span></b></a></div>
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<b class=""><span class="" style="font-size:16pt; font-family:"Helvetica Neue"">October 18-22, 2021 </span></b></div>
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<div class="" style="margin:0cm 0cm 0.0001pt"><font face="Helvetica Neue" size="3" class="">This is the final announcement for the 2021 HRMOS Science workshop, to be held from 9:00-13:00 CEST, 18-22 October, 2021.</font><font face="Helvetica Neue" size="3" class=""> </font></div>
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<div class="" style="margin:0cm 0cm 0.0001pt"><font face="Helvetica Neue" size="3" class="">Th</font><font size="3" class=""><font face="Helvetica Neue" class="">e </font><a href="https://protect-au.mimecast.com/s/wUXBCL7EwMfRDKZQqsq75pd?domain=indico.ict.inaf.it" class=""><b class="">Final
Program</b></a><font face="Helvetica Neue" class=""> fo</font></font><font face="Helvetica Neue" size="3" class="">r the meeting is attached and can be found at:</font></div>
<font face="Helvetica Neue" size="3" class=""><a href="https://protect-au.mimecast.com/s/wUXBCL7EwMfRDKZQqsq75pd?domain=indico.ict.inaf.it" class="">https://indico.ict.inaf.it/event/1547/timetable/#all.detailed</a></font>
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<div class="" style="margin:0cm 0cm 0.0001pt"><font face="Helvetica Neue" size="3" class="">The online connection details will be made available to the registered participants.</font><span class="" style="font-family:"Helvetica Neue"; font-size:12pt"> </span></div>
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<b class=""><span class="" style="font-family:"Helvetica Neue"">Registration</span></b><span class="" style="font-family:"Helvetica Neue"">:</span><u class=""><span class="" style="font-family:"Helvetica Neue"; color:rgb(70,135,255)"> <a href="https://protect-au.mimecast.com/s/scaHCMwGxOtqyXAzPtJxAFG?domain=indico.ict.inaf.it/" class="">https://indico.ict.inaf.it/event/1547/registrations</a></span></u><span class="" style="font-family:"Helvetica Neue""><a href="https://protect-au.mimecast.com/s/scaHCMwGxOtqyXAzPtJxAFG?domain=indico.ict.inaf.it/" class="">/</a><b class=""> </b></span></div>
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<b class=""><span class="" style="font-size:16pt; font-family:"Helvetica Neue"">Rationale </span></b><span class="" style="font-family:"Helvetica Neue"; font-size:12pt"> </span></div>
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<span class="" style="font-family:"Helvetica Neue"">The High-Resolution Multi-Object Spectrograph (HRMOS) is a proposed facility instrument for ESO’s VLT, following the initial presentation at the VLT 2030 workshop. HRMOS provides a combination of capabilities
essential to carry out breakthrough science across a broad range of active research areas from <b class="">Galactic and Local Group Archaeology to Stellar Astrophysics</b> <b class="">and Exoplanet </b>studies. HRMOS fills a gap in capabilities amongst the
landscape of future instrumentation planned for the next decade. The key capability of HRMOS is high spectral resolution (R = 60,000 - 80,000) with multi-object (50-100) capabilities and stability that provides radial velocity precision (~10m/s). Initial designs
predict a SNR=30 is achievable within 1hr for mag(AB) = 17-18 depending on resolution. The combination of high resolution and multiplex going to relatively bluer wavelengths (from 380nm), is truly a spectrograph that will push the boundaries of our knowledge
and is envisioned as a workhorse instrument in the future. </span></div>
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<span class="" style="font-family:"Helvetica Neue"">This conference aims to bring together the International scientific community, to propose and discuss science projects where HRMOS will have a strong impact due to its unparalleled capabilities, as well as
identifying the areas where it will provide unique synergies with existing and forthcoming large surveys and facilities such as 4MOST, WEAVE, MOONS and the ELTs. </span></div>
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<span class="" style="font-family:"Helvetica Neue"">This meeting is your opportunity to present your science with HRMOS and join the collaboration to push forward the HRMOS project in preparation for an upcoming White paper call.<b class=""> </b></span></div>
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<span class="" style="font-family:"Helvetica Neue"">For any questions, do not hesitate to contact Gayandhi, Sofia or Eline. </span></div>
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<span class="" style="font-family:"Helvetica Neue"">Best regards, </span></div>
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<span class="" style="font-family:"Helvetica Neue"">HRMOS Core Science Team </span></div>
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<span class="" style="font-family:"Helvetica Neue"; color:rgb(102,102,102)">Gayandhi De Sil</span><span class="" style="font-family:"Helvetica Neue"; color:rgb(102,102,102)">va </span><span class="" style="font-family:"Helvetica Neue"; color:rgb(95,95,95)">(AAO-Macquarie,
Australia), Sofia Randich (INAF-Arcetri, Italy), Eline Tolstoy (Kapteyn, The Netherlands), Laura Magrini (INAF-Arcetri, Italy), Vanessa Hill (OCA, France), Thomas Bensby (Lund, Sweden), Rob Jeffries (Keele, UK), Rodolfo Smiljanic (CAMK/PAN, Poland), Oscar
Gonzalez (UK-ATC, UK), Ása Skúladóttir (INAF-UNIFI, Italy), Nadège Largarde (UTINAM, Besançon, France) </span></div>
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<div class="" style="word-wrap:break-word">—</div>
<div class="" style="word-wrap:break-word">A/ Prof Gayandhi De Silva<br class="">
Australian Astronomical Optics, Macquarie University<br class="">
105 Delhi Rd, North Ryde, NSW 2113, Australia<br class="">
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<a href="mailto:gayandhi.desilva@mq.edu.au" class="">gayandhi.desilva@mq.edu.au</a></div>
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