2,435 research outputs found
The European VLBI network
The capabilities of the European very long baseline interferometry (VLBI) network are summarized. The range of baseline parameters, sensitivities, and recording and other equipment available are included. Plans for upgrading the recording facilities and the use of geostationary satellites for signal transfer and clock synchronization are discussed
The East-Asian VLBI Network
The East-Asian VLBI Network (EAVN) is the international VLBI facility in East
Asia and is conducted in collaboration with China, Japan, and Korea. The EAVN
consists of VLBI arrays operated in each East Asian country, containing 21
radio telescopes and three correlators. The EAVN will be mainly operated at 6.7
(C-band), 8 (X-band), 22 (K-band), and 43 GHz (Q-band), although the EAVN has
an ability to conduct observations at 1.6 - 129 GHz. We have conducted fringe
test observations eight times to date at 8 and 22 GHz and fringes have been
successfully detected at both frequencies. We have also conducted science
commissioning observations of 6.7 GHz methanol masers in massive star-forming
regions. The EAVN will be operational from the second half of 2017, providing
complementary results with the FAST on AGNs, massive star-forming regions, and
evolved stars with high angular resolution at cm- to mm-wavelengths.Comment: 6 pages, 3 figures, 2 tables. To appear in the proceedings of
"Frontiers in Radio Astronomy and FAST Early Sciences Symposium 2015" ed. Lei
Qian (ASP Conf. Ser.
Swift J1910.1-0546/MAXI J1910-057: e-EVN non-detection at 1.6 GHz
We observed the new transient Swift J1910.1-0546/MAXI J1910-057 with the European VLBI Network (EVN) in real-time mode on 12 June 2012. The observations were at 1.6 GHz and lasted for 4 hours
e-EVN detection of AGN activity in NGC 2617
NGC 2617 is a Seyfert 1.8 spiral galaxy at z=0.0142 (~60 Mpc, 1 mas = 0.3 pc) that is currently in outburst. We carried out European VLBI Network real-time e-VLBI observations at 1.6 GHz on 2013 June 7
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