evn:evn_science
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evn:evn_science [2018/09/12 09:44] – antonis | evn:evn_science [2021/05/03 07:30] (current) – kazi | ||
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- | [[http://www.jive.eu/ | + | [[https://www.evlbi.org|The next deadline is 1st of June 2021 16:00 UTC]]. |
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performed using multi-scale cleaning within the wsclean algorithm (Offringa et al. 2014). The total | 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 | 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 | + | extended (200-600 mas) gravitational |
- | excellent uv-coverage and surface brightness | + | excellent uv-coverage and surface brightness |
fundamental for a precise study of the structure of the extended arcs on mas-scales from | fundamental for a precise study of the structure of the extended arcs on mas-scales from | ||
MG J0751+2716. | MG J0751+2716. | ||
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These space-VLBI observations were obtained within the RadioAstron Nearby AGN Key Science Project coordinated by Tuomas Savolainen. 3C 84 was observed on September 21-22, 2013. In addition to SRT, more than two dozen ground radio telescopes, including the EVN, the KVN, Kalyazin and the NRAO VLBA, GBT and the phased JVLA participated in the experiment. First results are now published in Giovannini et al. (2018). | These space-VLBI observations were obtained within the RadioAstron Nearby AGN Key Science Project coordinated by Tuomas Savolainen. 3C 84 was observed on September 21-22, 2013. In addition to SRT, more than two dozen ground radio telescopes, including the EVN, the KVN, Kalyazin and the NRAO VLBA, GBT and the phased JVLA participated in the experiment. First results are now published in Giovannini et al. (2018). | ||
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**Figure:** Radio image of the central parsec in 3C 84 obtained with the space-VLBI array. The half- power-beam-width (HPBW) is 0.10 x 0.05 mas at PA 0o. The noise level is 1.4 mJy/beam and the peak intensity is 0.75 Jy/beam. The radio core and emission features C2 and C3 are indicated in the image. | **Figure:** Radio image of the central parsec in 3C 84 obtained with the space-VLBI array. The half- power-beam-width (HPBW) is 0.10 x 0.05 mas at PA 0o. The noise level is 1.4 mJy/beam and the peak intensity is 0.75 Jy/beam. The radio core and emission features C2 and C3 are indicated in the image. | ||
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evn/evn_science.txt · Last modified: 2021/05/03 07:30 by kazi