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<supportEmail caption="Support">evn2024@mpifr.de</supportEmail>
<title>16th European VLBI Network Symposium and Users' Meeting </title>
<description>&lt;h1&gt;The EVN Symposium&lt;/h1&gt;

&lt;p&gt;The European VLBI Network Symposium is the main forum for discussion of the latest Very Long Baseline Interferometry scientific results and technical and technological developments within the EVN member countries. The 16th EVN Symposium and Users meeting, hosted by the Max-Planck-Institut f&amp;uuml;r Radiostronomie, took place in Bonn in September 2-6, 2024.&lt;/p&gt;

&lt;p&gt;&lt;img alt="" src="https://events.mpifr-bonn.mpg.de/indico/event/371/picture/25.png" style="height:450px; width:600px" /&gt;&lt;/p&gt;

&lt;p&gt;&lt;em&gt;Informal group picture, taken on September 3, 2024 (Aleksei Nikonov)&lt;/em&gt;&lt;/p&gt;

&lt;p style="text-align:center"&gt;&lt;img alt="Poster thumbnail" src="https://events.mpifr-bonn.mpg.de/indico/event/371/picture/10.webp" style="height:452px; width:320px" /&gt;&lt;/p&gt;

&lt;p style="text-align:center"&gt;&lt;span style="font-size:11px"&gt;&lt;em&gt;Conference poster (for PDF version see the poster menu page).&lt;/em&gt;&lt;/span&gt;&lt;/p&gt;

&lt;p&gt;The covered topics included:&lt;/p&gt;

&lt;ul&gt;
	&lt;li&gt;Active galactic nuclei and relativistic outflows&lt;/li&gt;
	&lt;li&gt;Starburst galaxies, extragalactic masers, and supernovae&lt;/li&gt;
	&lt;li&gt;Stellar evolution and stellar masers&lt;/li&gt;
	&lt;li&gt;Transient sources and pulsars&lt;/li&gt;
	&lt;li&gt;Astrometric, geodetic &amp;amp; space applications of VLBI&lt;/li&gt;
	&lt;li&gt;VLBI technology developments&lt;/li&gt;
	&lt;li&gt;Users feedback&lt;/li&gt;
	&lt;li&gt;Current and future VLBI facilities and international cooperation&lt;/li&gt;
&lt;/ul&gt;

&lt;p&gt;Invited speakers:&lt;/p&gt;

&lt;ul&gt;
	&lt;li&gt;Markus Ackermann (DESY, Zeuthen, Germany)&lt;/li&gt;
	&lt;li&gt;Bia Boccardi (MPIfR, Bonn, Germany)&lt;/li&gt;
	&lt;li&gt;Roger Deane (University of Witwatersrand, Johannesburg, South Africa)&lt;/li&gt;
	&lt;li&gt;Simon Garrington (Jodrell Bank Observatory, Manchester, United Kingdom)&lt;/li&gt;
	&lt;li&gt;Giancarlo Ghirlanda (Osservatorio di Brera, Milano, Italy)&lt;/li&gt;
	&lt;li&gt;Preeti Kharb (Tata Institute for Fundamental Research, Pune, India)&lt;/li&gt;
	&lt;li&gt;Michela Mapelli (Universit&amp;auml;t Heidelberg, Germany)&lt;/li&gt;
	&lt;li&gt;Benito Marcote (Joint Institute for VLBI-ERIC, Dwingeloo, The Netherlands)&lt;/li&gt;
	&lt;li&gt;James Miller-Jones (Curtin University, Melbourne, Australia)&lt;/li&gt;
	&lt;li&gt;Suma Murthy&amp;nbsp;(Joint Institute for VLBI-ERIC, Dwingeloo, The Netherlands)&lt;/li&gt;
	&lt;li&gt;Alexander Plavin (Harvard-Smithsonian Centre for Astrophysics, Cambridge, MA, USA)&lt;/li&gt;
	&lt;li&gt;Eduardo Ros (MPIfR, Bonn, Germany)&lt;/li&gt;
	&lt;li&gt;Gabriele Surcis (Osservatorio di Cagliari, Italy)&lt;/li&gt;
	&lt;li&gt;Kiyoaki Wajima (KASI Daejeon, Korea &amp;amp; Shanghai Observatory, PR China)&lt;/li&gt;
	&lt;li&gt;Benjamin Winkel (MPIfR, Bonn, Germany)&lt;/li&gt;
	&lt;li&gt;Simona Vegetti (MPA, Garching, Germany)&lt;/li&gt;
	&lt;li&gt;Jun Yang (Chalmers University of Technology, G&amp;ouml;teborg, Sweden)&lt;/li&gt;
&lt;/ul&gt;

&lt;p&gt;Scientific Organising Committee:&lt;/p&gt;

&lt;ul&gt;
	&lt;li&gt;Tao An (Shanghai Observatory, China)&lt;/li&gt;
	&lt;li&gt;Pikky Atri (ASTRON, Dwingeloo, Netherlands)&lt;/li&gt;
	&lt;li&gt;Paola Castangia (INAF Cagliari, Italy)&lt;/li&gt;
	&lt;li&gt;Talvikki Hovatta (Aalto University, Espoo, Finland)&lt;/li&gt;
	&lt;li&gt;Marcin Gawroński (University of Torun, Poland)&lt;/li&gt;
	&lt;li&gt;Michael Lindqvist (Onsala Space Observatory, Sweden)&lt;/li&gt;
	&lt;li&gt;Andrei Lobanov (MPIfR, Bonn, Germany; chair)&lt;/li&gt;
	&lt;li&gt;Sara Motta (INAF Milano, Italy)&lt;/li&gt;
	&lt;li&gt;Tom Muxlow (University of Manchester, UK)&lt;/li&gt;
	&lt;li&gt;Zsolt Paragi (JIV-ERIC, Dwingeloo, Netherlands)&lt;/li&gt;
	&lt;li&gt;Kazi Rygl (INAF Bologna, Italy)&lt;/li&gt;
&lt;/ul&gt;

&lt;p&gt;Local Organising Committee:&lt;/p&gt;

&lt;ul&gt;
	&lt;li&gt;Si&amp;acirc;n Adey&lt;/li&gt;
	&lt;li&gt;Vieri Bartolini&lt;/li&gt;
	&lt;li&gt;Petra Benke&lt;/li&gt;
	&lt;li&gt;Lena Debbrecht&lt;/li&gt;
	&lt;li&gt;Sergio Dzib-Quijano&lt;/li&gt;
	&lt;li&gt;JongSeo Kim&lt;/li&gt;
	&lt;li&gt;Galina Lipunova&lt;/li&gt;
	&lt;li&gt;Andrei P. Lobanov&lt;/li&gt;
	&lt;li&gt;Jan R&amp;ouml;der&lt;/li&gt;
	&lt;li&gt;Eduardo Ros (chair)&lt;/li&gt;
	&lt;li&gt;Saurabh&lt;/li&gt;
&lt;/ul&gt;

&lt;p&gt;Conference proceedings will be published as result of the conference presentations and discussion (see the menu to the left).&amp;nbsp; Stay tuned for more information!&lt;/p&gt;

&lt;h2&gt;&lt;img alt="" src="https://events.mpifr-bonn.mpg.de/indico/event/371/picture/0.png" style="height:82px; width:700px" /&gt;&lt;/h2&gt;
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<location>
 <name>CJD Bonn Castell</name>
 <address>Graurheindorfer Str. 149, 53117 Bonn</address>
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<startDate>2024-09-02T09:00:00</startDate>
<endDate>2024-09-06T15:00:00</endDate>
<creationDate>2023-11-22T16:57:26</creationDate>
<modificationDate>2024-12-30T17:22:04</modificationDate>
<timezone>Europe/Berlin</timezone>
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 <title>The nature of the radio host galaxy of the QPE source RXJ1301.9+2747</title>
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   <name first="Sebastiano Daniel" middle="" last="von Fellenberg"></name>
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  <name>CJD Bonn Castell</name>
  <address>Graurheindorfer Str. 149, 53117 Bonn</address>
  <room></room>
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 <duration>00:20</duration>
 <abstract>Quasi-periodic eruptions are repeating burst of X-ray emission, that occur roughly periodically on time intervals of a few hours. Only 6 QPE source were so far detected. While the underlying mechanism for the observed X-ray emission is not fully understood, it is generally believed to be caused be the interaction between a star or stellar remnant with the accretion disk of a super massive black hole, potentially related to partial Tidal Disruption Events (pTDEs). 

The some of the host galaxies of QPEs are detected in radio, and share that they are faint (few tenths of micro-Jansky). Here, we report on new HSA observations of the RXJ1301.9+2747 at 5GHz, which sheds light on the nature of the radio emission of the host galaxy.</abstract>
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