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--- evn:evn_science [2018/09/12 09:45] – [Space-VLBI observations resolve the edge-brightened jet in 3C 84 (NGC1275) at 30 microarcseconds from the core] antonis
+++ evn:evn_science [2020/12/21 09:54] – [Introduction] kazi
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-{{ :evn:worldmap.jpeg?800 |}}
+{{ :evn:worldmap.jpeg?600 |}}
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-[[http://www.jive.eu/jivewiki/doku.php?id=evn:guidelines|The next deadline is October 1, 2018]].
+[[https://www.evlbi.org|The next deadline is 1st of February 2021 16:00 UTC]].
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 performed using multi-scale cleaning within the wsclean algorithm (Offringa et al. 2014). The total
 flux density of the target is 350 mJy and the off-source rms is 41 μJy/beam. Never before have such
-extended (200-600 mas) gravitaTonal arcs been detected at an angular resoluTon of a few mas. The
+extended (200-600 mas) gravitational arcs been detected at an angular resoluTon of a few mas. The
-excellent uv-coverage and surface brightness sensiTvity provided by the global VLBI array have been
+excellent uv-coverage and surface brightness sensitivity provided by the global VLBI array have been
 fundamental for a precise study of the structure of the extended arcs on mas-scales from
 MG J0751+2716.
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