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--- evn:evn_science [2018/09/12 09:12] – antonis
+++ evn:evn_science [2018/09/12 09:15] – antonis
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 =====Gravitationally-lensed radio arcs observed with global VLBI=====
-[[https://doi.org/10.1093/mnras/sty1326|Spingola et al (2018)]]
 The Strong lensing at High Angular ResoluTon Program (SHARP) led by McKean (ASTRON) has
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 show extended arcs on VLBI-scales. The global VLBI L-band deep imaging detects all of the extended
 arcs at high significance, showing the complex surface brightness structure of the background
-source in unprecedented detail (see Figure). Because of the complexity of this system, the imaging was
+source in unprecedented detail (see Figure from [[https://doi.org/10.1093/mnras/sty1326|Spingola et al (2018)]]). Because of the complexity of this system, the imaging was
 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
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 MG J0751+2716.
-{{:evn:grav_lens_spingola.jpeg?200|}}
+{{:evn:grav_lens_spingola.jpeg?400|}}
 **Figure 1.**Global VLBI imaging of MG J0751+2716 at 1.65 GHz (Spingola et al. (2018)). The off-source
 rms is 41 μJy/beam and the peak surface brightness is 2.9 mJy/beam. The restored beam is 5.5x1.8