Differences
This shows you the differences between two versions of the page.
Both sides previous revisionPrevious revisionNext revision | Previous revisionNext revisionBoth sides next revision |
evn:evn_publications [2020/04/23 19:36] – kazi | evn:evn_publications [2020/12/21 09:53] – kazi |
---|
\\ | \\ |
\\ | \\ |
The [[http://www.evlbi.org/|European VLBI Network (EVN)]] is a VLBI network of radio telescopes in Europe and beyond, operated by an international Consortium of institutes. The EVN operates an “open sky” policy and observing proposals are accepted (and peer-reviewed) from astronomers from all over the world. [[https://www.evlbi.org|The next deadline is June 1, 2020]]. | The [[http://www.evlbi.org/|European VLBI Network (EVN)]] is a VLBI network of radio telescopes in Europe and beyond, operated by an international Consortium of institutes. The EVN operates an “open sky” policy and observing proposals are accepted (and peer-reviewed) from astronomers from all over the world. [[https://www.evlbi.org|The next deadline is 1st of February 2021 16:00 UTC]]. |
| |
| |
2019 | 2019 |
| |
* Surcis G., Vlemmings W.H.T., van Langevelde H.J., et al.\\ A&A 623, A130, 2019 | * {{:evn:evn_publications_2019.pdf|EVN publications 2019}} |
* [[https://doi.org/10.1051/0004-6361/201834578|EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions. IV. Magnetic field strength limits and structure for seven additional sources]] | |
| |
* Cau H., Frey S., Gabanyi K., et al.\\ MNRAS 482, L34, 2019 | |
* [[https://doi.org/10.1093/mnrasl/sly184|The loud and the quiet: searching for radio counterparts of two radio-weak BL Lac candidates with VLBI]] | |
| |
* Yang J., An T., Zheng F., et al.\\ MNRAS 482, 1701, 2019 | |
* [[https://doi.org/10.1093/mnras/sty2798|A radio structure resolved at the deca-parsec scale in the radio-quiet quasar PDS 456 with an extremely powerful X-ray outflow]] | |
| |
| |