<div dir="ltr"><div><div><font face="arial, sans-serif" color="#000000">Dear all,</font></div><div><font face="arial, sans-serif" color="#000000"><br></font></div><div><font face="arial, sans-serif" color="#000000">[Apologies if you receive this email multiple times.]</font></div><div><font face="arial, sans-serif" color="#000000"><br></font></div><div><font face="arial, sans-serif" color="#000000">As you may be well-aware, given numerous emails, we are now less than 3 weeks away from the <b>1st-March-2024 deadline (<a href="https://protect-au.mimecast.com/s/HvY-COMKzVTNV9407SEGvv9?domain=astronomy2024.org/" target="_blank">https://astronomy2024.org/abstracts-grants/</a>)</b> for:</font></div><span class="gmail-im" style=""><font color="#000000"><div><font face="arial, sans-serif">* Submitting abstracts for the IAU General Assembly in Cape Town (GA2024) </font></div><div><font face="arial, sans-serif">* Applying for a grant, to support participation in GA2024</font></div><div><font face="arial, sans-serif">* Registering to qualify for the Early-Bird registration fee (<a href="https://protect-au.mimecast.com/s/wSliC3QNPBiX1J0GyS9r-eA?domain=astronomy2024.org" target="_blank">https://astronomy2024.org/registration/</a>)</font></div><div><font face="arial, sans-serif"><br></font></div><div><b><font face="arial, sans-serif">We invite you to our IAU symposium, which is catered specifically for studies of active galactic nuclei (AGN), and titled: 'All-inclusive AGN' (<a href="https://protect-au.mimecast.com/s/aeHSCQnMBZfXGEr32SM24VG?domain=allinclusiveagn.saao.ac.za/" target="_blank">https://allinclusiveagn.saao.ac.za/</a>).</font></b></div><div><font face="arial, sans-serif"><br></font></div><div><font face="arial, sans-serif">'AGN' is a key research topic in galaxy evolution, given the abundance of evidence that suggests a cause-and-effect relationship between galaxies and the supermassive black-holes at their cores. We will discuss the latest results in observation- and simulation-driven studies, covering both multi-wavelength and multi-messenger astronomy over a wide range of spatial scales and timescales. In particular, we will showcase work that uses southern-hemisphere telescopes such as <a href="https://protect-au.mimecast.com/s/3N2OCROND2uG9kBRMuOfVdL?domain=sarao.ac.za/" target="_blank" style="box-sizing:inherit;text-decoration-line:none">MeerKAT</a>, <a href="https://protect-au.mimecast.com/s/zO3gCVARKgC2rL95WcQTUDy?domain=saao.ac.za/" target="_blank" style="box-sizing:inherit;text-decoration-line:none">SALT</a>, <a href="https://protect-au.mimecast.com/s/wZggCWLVXkU67gGPMSpjbVu?domain=mpi-hd.mpg.de/" target="_blank" style="box-sizing:inherit;text-decoration-line:none">H.E.S.S.</a>, <a href="https://protect-au.mimecast.com/s/MvJ9CXLW2mU4vy0q8I70A_x?domain=almaobservatory.org/" target="_blank" style="box-sizing:inherit;text-decoration-line:none">ALMA</a>, and the <a href="https://protect-au.mimecast.com/s/arMJCYW8NocDRJONnTj-xMr?domain=eso.org/" target="_blank" style="box-sizing:inherit;text-decoration-line:none">VLT</a>, in addition to exciting, new observations from <a href="https://protect-au.mimecast.com/s/ehVPCZY1Nqi7ZV2DkFMaTcB?domain=webb.nasa.gov" target="_blank" style="box-sizing:inherit;text-decoration-line:none">JWST</a>, <a href="https://protect-au.mimecast.com/s/dpYwC1WLPxc6yD5kPSAVBXm?domain=eventhorizontelescope.org/" target="_blank" style="box-sizing:inherit;text-decoration-line:none">EHT</a>, and the <a href="https://protect-au.mimecast.com/s/VbtDC2xMQziVqJORBtpFYR4?domain=rubinobservatory.org/" target="_blank" style="box-sizing:inherit;text-decoration-line:none">Vera C. Rubin Observatory</a>. Furthermore, we will incorporate a discussion on equity, diversity, and inclusion (EDI) in Astronomy — which is pivotal for the whole community — because researchers may not commonly set aside time to participate in EDI talks or see the relevance of EDI initiatives. </font></div><div><font face="arial, sans-serif"><br></font></div><div><b><font face="arial, sans-serif">Topics included:</font></b></div><div><ul style="box-sizing:border-box;margin:0px;padding:0px;list-style-position:initial"><li style="margin-left:15px"><font face="arial, sans-serif">Co-evolution of AGN and their host galaxies</font></li><li style="margin-left:15px;box-sizing:inherit"><font face="arial, sans-serif">Multiwavelength AGN studies and future observing facilities</font></li><li style="margin-left:15px;box-sizing:inherit"><font face="arial, sans-serif">Simulations of AGN, host galaxies and their gas environments</font></li><li style="margin-left:15px;box-sizing:inherit"><font face="arial, sans-serif">Time-domain studies of AGN (e.g. reverberation mapping)</font></li><li style="margin-left:15px;box-sizing:inherit"><font face="arial, sans-serif">Multimessenger astrophysics connected to AGN (e.g. gravitational waves, neutrinos)</font></li><li style="margin-left:15px"><font face="arial, sans-serif">AGN classification and unification models</font></li><li style="margin-left:15px"><font face="arial, sans-serif">Mechanical and radiative AGN feedback mechanisms</font></li><li style="margin-left:15px"><font face="arial, sans-serif">The intergalactic and circumgalactic medium (IGM/CGM) of AGN host galaxies</font></li><li style="margin-left:15px"><font face="arial, sans-serif">Star formation and molecular gas in AGN host galaxies</font></li><li style="margin-left:15px"><font face="arial, sans-serif">The evolution of AGN at high redshift</font></li></ul></div><div><font face="arial, sans-serif"><br></font></div><div><b><font face="arial, sans-serif">Our confirmed, invited speakers and panel-members include:</font></b></div><div><font face="arial, sans-serif">Prof. Roberto J. Assef [he] (Universidad Diego Portales, Chile)</font></div><div><font face="arial, sans-serif">Dr Beatriz Mingo [she] (The Open University, UK)</font></div><div><font face="arial, sans-serif">Dr Dylan Nelson [he] (University of Heidelberg, Germany)</font></div></font></span><div><font face="arial, sans-serif" color="#000000">Dr Nicole Thomas [she] (University of Western Australia, Australia)</font></div><div><span style="color:rgb(0,0,0);font-family:arial,sans-serif">Dr Jan Scholtz [he] (Kavli Institute for Cosmology (Cambridge), UK)</span></div><div><div class="gmail-im" style=""><div><font face="arial, sans-serif" color="#000000">Prof. Jarita Holbrook [she] (The University of Edinburgh, UK)</font></div><div><font face="arial, sans-serif" color="#000000">Prof. Debra Meyer [she] (The University of Johannesburg, South Africa)</font></div><div><font face="arial, sans-serif" color="#000000">Prof. Prajval Shastri [she] (Raman Research Institute, India)</font></div><div><font face="arial, sans-serif" color="#000000">Dr Alfredo Carpineti [he] (Chair & Founder of ‘Pride in STEM’)</font></div><div><font face="arial, sans-serif" color="#000000"><br></font></div><div><div><span id="m_-8072078829034407741m_-6888249083108654189m_-4688444439006057058m_505029641359186141gmail-docs-internal-guid-85d553bf-7fff-a1ea-d440-cc5c05d8f5ae"><font face="arial, sans-serif" color="#000000"><p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">and we look forward to your contributions towards addressing the many open and unanswered questions that have been discussed widely in the literature, such as: </span></p><br><p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-style:italic;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">AGN feedback</span></p><ul style="margin-top:0px;margin-bottom:0px"><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">What is the role of jets in driving AGN outflows? How do outflows evolve?</span></p></li><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">What are relativistic jets composed of and what powers their acceleration?</span></p></li><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">How do radio jets, outflows, and radiative processes interact with their host galaxies and galaxy haloes?</span></p></li></ul><br><p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-style:italic;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">Black-hole feeding and accretion</span></p><ul style="margin-top:0px;margin-bottom:0px"><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">How does the fuelling gas reach the innermost region of the AGN? </span></p></li><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">What are the causes and observables of extreme AGN variability?</span></p></li></ul><ul style="margin-top:0px;margin-bottom:0px"><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">What is the AGN X-ray corona’s origin and structure?</span></p></li></ul><br><p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><i>The torus and dust obscuration</i></span></p><ul style="margin-top:0px;margin-bottom:0px"><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">What is the structure and composition of the dusty torus?</span></p></li><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">How is accretion flow affected by the torus?</span></p></li></ul><br><p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-style:italic;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">Properties of the host galaxies</span></p><ul style="margin-top:0px;margin-bottom:0px"><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">Which AGN processes produce the various emission lines observed?</span></p></li><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">How does the morphology, stellar populations, dust and metallicity of a galaxy co-evolve with the AGN? </span></p></li></ul><br><p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-style:italic;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">The ISM, IGM, and CGM</span></p><ul style="margin-top:0px;margin-bottom:0px"><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">What is the interplay between accretion, star formation and the ISM in the host galaxies?</span><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"> </span></p></li><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">How does AGN feedback affect the observable properties of the IGM and CGM?</span></p></li><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">How is gas accretion from the CGM, or directly from the IGM, affected by the physics of the ISM and by AGN feedback?</span></p></li></ul><p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-style:italic;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"> </span></p><p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><i>AGN population studies</i></span></p><ul style="margin-top:0px;margin-bottom:0px"><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">How is gravitational-wave astrophysics affecting our understanding of AGN?</span></p></li><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">Are AGN an important astrophysical source of high-energy neutrinos?</span></p></li><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">What is the typical variability of AGN and how can we improve reverberation mapping of AGN?</span></p></li></ul><br><p dir="ltr" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="background-color:transparent;font-style:italic;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">Cosmic evolution of AGN</span></p><ul style="margin-top:0px;margin-bottom:0px"><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">How were black holes of the highest-redshift AGN formed?</span></p></li><li dir="ltr" style="margin-left:15px;list-style-type:disc;background-color:transparent;font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline"><p dir="ltr" role="presentation" style="line-height:1.38;margin-top:0pt;margin-bottom:0pt"><span style="font-variant-numeric:normal;font-variant-east-asian:normal;font-variant-alternates:normal;vertical-align:baseline">What role did AGN play during the Epoch of Reionisation?</span></p></li></ul></font></span></div></div><div><font face="arial, sans-serif" color="#000000"><br></font></div></div></div><div><font face="arial, sans-serif" color="#000000">This symposium is an excellent 5-year follow-up to the IAU Symposium held in Ethiopia on “Nuclear activity in galaxies across cosmic time”, and so will continue to establish and develop international collaborations across and beyond the African continent. For this to be successful, we need you and your <i>active</i> engagement! [ If you pardon the pun ;) ]</font></div><div><font face="arial, sans-serif" color="#000000"><br></font></div><div class="gmail-adL"><div class="gmail-im" style=""><div style=""><b><font face="arial, sans-serif" color="#000000">We very much look forward to seeing you at 'All-inclusive AGN', either in-person or online.</font></b></div><div style=""><font face="arial, sans-serif" color="#000000"><br></font></div><div style=""><b><font face="arial, sans-serif" color="#000000">Best wishes,</font></b></div><div style=""><b><font face="arial, sans-serif" color="#000000">Sarah and Sthabile</font></b></div><div style=""><b><font face="arial, sans-serif" color="#000000"><br></font></b></div><div style=""><font face="arial, sans-serif" color="#000000"><b>on behalf of the 'All-inclusive AGN' SOC:</b></font></div><div style=""><font face="arial, sans-serif" color="#000000"><span style="box-sizing:inherit"><i>Chair</i>:</span> Dr Sarah V. White [she] (South African Astronomical Observatory [SAAO], South Africa)<br><span style="box-sizing:inherit"><i>Vice-Chair</i>: </span>Dr Sthabile Kolwa [they/she] (University of Johannesburg, South Africa)<br>Prof. Tao An [he] (Shanghai Astronomical Observatory [SHAO], China)<br>Prof. Sara Ellison [she] (University of Victoria, Canada)<br>Assoc. Prof. Preeti Kharb [she] (National Centre for Radio Astrophysics [NCRA], India)<br>Dr Vincenzo Mainieri [he] (European Southern Observatory [ESO], Germany)<br>Prof. Roberto Maiolino [he] (University of Cambridge, UK)<br>Dr Lucia Marchetti [she] (University of Cape Town, South Africa) – IAU Division-J representative<br>Dr Andrea Merloni [he] (Max Planck Institute for Extraterrestrial Physics [MPE], Germany)<br>Assoc. Prof. Leah Morabito [she] (Durham University, UK)<br>Dr Roderik Overzier [he] (Observatório Nacional, Brazil)<br>Dr Annalisa Pillepich [she] (Max Planck Institute for Astronomy [MPiA], Germany)<br>Prof. Mirjana Pović [she] (Space Science & Geospatial Institute [SSGI], Ethiopia/IAA-CSIC, Spain)<br>Prof. Elaine Sadler [she] (University of Sydney and CSIRO, Australia)<br>Assoc. Prof. Stas Shabala [he] (University of Tasmania, Australia)<br>Dr Daniel Stern [he] (Jet Propulsion Laboratory [JPL]/California Institute of Technology, US) <br>Assoc. Prof. Ryan Trainor [he] (Franklin & Marshall College, US)</font></div></div></div></div><br clear="all"><div><div dir="ltr" class="gmail_signature" data-smartmail="gmail_signature"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><div dir="ltr"><p style="margin-top:0px;margin-bottom:0px"><font size="2" face="arial, helvetica, sans-serif" color="#666666">----------------------------------------------------------------------------------------------------</font></p><p style="margin-top:0px;margin-bottom:0px"><font face="arial, sans-serif"><font size="2" color="#666666">Dr Sarah White (she/her), </font><a href="https://protect-au.mimecast.com/s/QXihC4QOPEizNQ3mDso2sA3?domain=astronomersforplanet.earth" style="color:rgb(17,85,204)" target="_blank">astronomersforplanet.earth</a></font></p><p style="margin-top:0px;margin-bottom:0px"><font color="#666666" face="arial, sans-serif">Astronomer (<a href="mailto:sarahwhite.astro@gmail.com" target="_blank">sarahwhite.astro@gmail.com</a> , <a href="mailto:sarah.white@saao.ac.za" target="_blank">sarah.white@saao.ac.za</a>)</font></p><p style="margin-top:0px;margin-bottom:0px"><font color="#666666">South African Astronomical Observatory (SAAO), </font></p><p style="margin-top:0px;margin-bottom:0px"><font color="#666666">P.O. Box 9, Observatory, 7935<span style="font-family:arial,sans-serif">, South Africa.</span></font></p><p style="margin-top:0px;margin-bottom:0px;color:rgb(0,0,0)"><br></p></div></div></div></div></div></div></div></div></div></div></div></div></div></div></div></div></div></div></div></div></div></div>