e-EVN status table
Advertised frequencies and array configurations
Frequency band |
e-EVN + e-MERLIN array |
1.6-1.4 GHz (18-21cm) |
Ar, Ir, Ef, Hh, Jb, Mc, Nt, On85, T6/Sh, Tr, Wb1, (Bd, Sv, Zc)*, Cm, Da, De, Kn, Pi |
5 GHz (6cm) |
Ar, Ir, Ef, Hh, Jb, Mc, Nt, On85, T6/Sh, Tr, Ys, Wb1, (Bd, Sv, Zc)*, Cm, Da, De, Kn, Pi |
6 GHz (5cm) |
Ar, Ir, Ef, Hh, Jb, Mc, Nt, On85, Tr, Ys, Wb1, (Bd, Sv, Zc)*, Cm, Da, De, Kn, Pi |
22 GHz (1.3cm) |
Ef, Hh, Jb, Mc, Mh, Nt, On60, Sh, Tr, Ys, (Bd, Sv, Zc)*, Cm, Da, De, Kn, Pi |
The phased-array WSRT is no longer vailable, only a single dish.
*The Quasar stations may be available for some of the e-EVN runs with a limited data rate (likely 1 Gbit/s).
The following telescopes have been upgraded to 2 Gbit/s: Ef, Hh, Jb, Mc, Nt, On, Sh, Ys, Tr, Wb1 (due to
a limitation in the IF system, Wb1 only has a bandwidth of 160 MHz). Still limited to 1 Gbit/s: Mh.
Arecibo is limited to 512 Mbit/s without UT restriction (as from October 2013),
up to 72 hours per month.
e-MERLIN outstations (Cm, Da, De, Kn, Pi) are limited to 512 Mbps.
Mixed-bandwidth observations are possible.
The current limitation for real-time e-VLBI correlation is estimated to be
8 telescopes at 2 Gbit/s, or 15 telescopes at 1 Gbit/s. For example, 6 stations
at 2 Gbit/s + 3 stations at 1 Gbit/s, or 5 stations at 2 Gbit/s and 4 stations
at 1 Gbit/s should be possible.
Scheduled e-EVN runs
19 June 2018, 13:00 UTC |
6:51 GST |
20 June 2018, 13:00 UTC |
6:55 GST |
18 September 2018, 13:00 UTC |
12:50 GST |
19 September 2018, 13:00 UTC |
12:54 GST |
16 October 2018, 13:00 UTC |
14:40 GST |
17 October 2018, 13:00 UTC |
14:44 GST |
20 November 2018, 13:00 UTC |
16:58 GST |
21 November 2018, 13:00 UTC |
17:02 GST |
4 December 2018, 13:00 UTC |
17:53 GST |
5 December 2018, 13:00 UTC |
17:57 GST |
22 January 2019, 13:00 UTC |
21:06 GST |
23 January 2019, 13:00 UTC |
21:10 GST |
14 February 2019, 13:00 UTC |
22:37 GST |
15 February 2019, 13:00 UTC |
22:41 GST |
19 March 2019, 13:00 UTC |
0:47 GST |
20 March 2019, 13:00 UTC |
0:51 GST |
16 April 2019, 13:00 UTC |
2:38 GST |
17 April 2019, 13:00 UTC |
2:41 GST |
14 May 2019, 13:00 UTC |
4:28 GST |
15 May 2019, 13:00 UTC |
4:32 GST |
18 June 2019, 13:00 UTC |
6:46 GST |
19 June 2019, 13:00 UTC |
6:50 GST |
17 September 2019, 13:00 UTC |
12:45 GST |
18 September 2019, 13:00 UTC |
12:49 GST |
15 October 2019, 13:00 UTC |
14:35 GST |
16 October 2019, 13:00 UTC |
14:39 GST |
12 November 2019, 13:00 UTC |
16:25 GST |
13 November 2019, 13:00 UTC |
16:29 GST |
3 December 2019, 13:00 UTC |
17:48 GST |
4 December 2019, 13:00 UTC |
17:52 GST |
The observing frequency in a session is decided based on proposal pressure
* Not advertised e-VLBI date; ToO or within regular EVN session
#! cancelled e-VLBI date