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<category>Conferences</category>
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  <title>Prof.</title>
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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;
</description>
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<closed>False</closed>
<location>
 <name>CJD Bonn Castell</name>
 <address>Graurheindorfer Str. 149, 53117 Bonn</address>
 <room></room>
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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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 <user>
  <title>Dr.</title>
  <name first="Andrei" middle="" last="Lobanov"></name>
  <organization></organization>
  <emailHash>4dffa7689a6089770a09283de01dfe1c</emailHash>
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 <user>
  <title>Prof.</title>
  <name first="Eduardo" middle="" last="Ros"></name>
  <organization></organization>
  <emailHash>6c9e606df0845ea84b327fc5f7fd6dee</emailHash>
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 <title>The faint radio nucleus of the megamaser galaxy IC485: AGN or SF activity?</title>
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   <title>Dr.</title>
   <name first="Paola" middle="" last="Castangia"></name>
   <organization>INAF - Osservatorio Astronomico di Cagliari</organization>
   <emailHash>be1ccf56d8958fc774089324e30b8c19</emailHash>
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  <user>
   <title>Dr.</title>
   <name first="Paola" middle="" last="Castangia"></name>
   <organization>INAF - Osservatorio Astronomico di Cagliari</organization>
   <emailHash>be1ccf56d8958fc774089324e30b8c19</emailHash>
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   <title>Mrs.</title>
   <name first="Elisabetta" middle="" last="Ladu"></name>
   <organization>INAF - Osservatorio Astronomico di Cagliari</organization>
   <emailHash>3b00879a5f997522d15d9f1ca06a64f1</emailHash>
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   <title>Dr.</title>
   <name first="Andrea" middle="" last="Tarchi"></name>
   <organization>INAF - Osservatorio Astronomico di Cagliari</organization>
   <emailHash>9b29a98b06d82ed6fac6f3b97555cdf0</emailHash>
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   <title>Dr.</title>
   <name first="Gabriele" middle="" last="Surcis"></name>
   <organization>INAF - Osservatorio Astronomico di Cagliari</organization>
   <emailHash>eda0afb8da7cf4f96e288bf51df3d494</emailHash>
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   <title>Dr.</title>
   <name first="David" middle="" last="Williams-Baldwin"></name>
   <organization>Jodrell Bank Centre for Astrophysics</organization>
   <emailHash>2bf6ce5f382dab2780d548a1402208e3</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Francesca" middle="" last="Panessa"></name>
   <organization>INAF - IAPS Roma</organization>
   <emailHash>f1ee52e95b7606fd62511e2f463b6eff</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="James" middle="" last="Braatz"></name>
   <organization>NRAO</organization>
   <emailHash>09b7989d795f168a6e7f2a0fc0a43d40</emailHash>
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   <title>Dr.</title>
   <name first="Dominic" middle="" last="Pesce"></name>
   <organization>CfA</organization>
   <emailHash>444eaa4ce92b203295a7de481f3ce763</emailHash>
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 </coAuthors>
 <location>
  <name>CJD Bonn Castell</name>
  <address>Graurheindorfer Str. 149, 53117 Bonn</address>
  <room></room>
 </location>
 <startDate>2024-09-03T11:45:00</startDate>
 <endDate>2024-09-03T12:00:00</endDate>
 <duration>00:15</duration>
 <abstract>Water masers associated with AGNs (the `megamasers') constitute a unique way to directly map the molecular gas at (sub-)parsec distance from SMBHs and, hence, to study the physical properties, the structure, and the kinematics of the gas surrounding the central engine. In particular, high angular resolution radio continuum and maser observations have been used to test the alignment of the radio jets and the rotation axis of accretion disks and to pinpoint regions of strong interaction of low power jets and/or nuclear outflows with the interstellar medium in radio quiet AGNs.

Located at a distance of 122 Mpc, IC485 is a spiral LINER/Seyfert 2 galaxy hosting a bright H2O megamaser. A recent study indicates that the maser emission might be produced (at least in part) in an edge-on accretion disk oriented north-south, with a radius of 0.24 pc (Ladu et al. 2024). Sensitive radio continuum EVN measurements at 1.7 and 5 GHz, did not show confident emission from the nuclear region, suggesting a diffuse morphology resolved out at the pc-scale. 

By taking profit of a resolution intermediate between that of the VLA and VLBI, very recent observations with the e-MERLIN at 1.4 and 5 GHz revealed a flat-spectrum nuclear source, coincident in position with the maser location and with a tentative source visible in our EVN L-band map. The e-MERLIN source is slightly resolved with an orientation of the extended emission approximately perpendicular to that of the putative accretion disk. These characteristics suggest the presence of a weak jet or an outflow in the nucleus of IC485. Here, we present the results of our e-MERLIN observations and discuss them by combining the information obtained from the radio continuum and maser studies, thus providing relevant clues on the maser and radio continuum origin.</abstract>
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