e-VLBI with LOFAR
O. Wucknitz
- Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany
Abstract
LOFAR for the first time offers the possibility to image the radio
sky at wavelengths of a few metres with a resolution in the arcsec range or
better. This is made possible by international stations that provide
baselines of several hundred km and turn LOFAR into an e-VLBI array. In
this talk I give an overview of first high-resolution observations using the
International LOFAR Telescope and discuss the particular challenges of
long-baseline LOFAR observations.
In addition the first resolved LOFAR images of the Sun are presented.
PoS (10th EVN Symposium) (2010) 050 (link to online journal)
download original presentation
PDF file (4.5 MB, last change 30 Sep 2010)
43 pages, suitable for presentation with acroread. This
version also included hyperlinks for quick navigation and external links
to movies.
download printable version (small)
PDF file (1.8 MB, last change 30 Sep 2010)
Paper saving version. 5 pages, text in b/w, colour figures. 8 slides per A4 page.
download proceedings version
PDF file (1.9 MB, last change 16 Nov 2010)
6 pages
download movie 1: single-band delay/rate 3C196 20 Aug 2009, DE-NL
GIF file (700.0 kB, last change 29 Sep 2009)
download movie 2: coherent multi-band delay/rate 3C196 20 Aug 2009, DE-NL
GIF file (1.1 MB, last change 29 Sep 2009)
download movie 3: incoherent multi-band delay/rate 3C196 Unterweilenbach-Tautenburg
MPEG4 movie (8.2 MB, last change 16 Feb 2010)
download movie 4: the Sun with 1 sec integration time per step, real duration 30
sec, about 10:17:10 - 10:17:40 on 9-Jun-2010, plays in real-time
MPEG4 movie (129.9 kB, last change 8 Jul 2010)
download movie 5 (additional material): the Sun with 10 sec integration time per step, real duration ca. 10
min, about 10:16:30 - 10:26:20 on 9-Jun-2010, plays 100 times
faster than real-time
MPEG4 movie (176.3 kB, last change 8 Jul 2010)
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Script last modified on 7 Sep 2010
Last change to this data base entry on 26 May 2011