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<!DOCTYPE article SYSTEM "http://www.adv-radio-sci.net/inc/ars/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Advances in Radio Science</journal_title>
		<journal_url>www.adv-radio-sci.net</journal_url>
		<issn>1684-9965</issn>
		<eissn>1684-9973</eissn>
		<volume_number>5</volume_number>
		<volume_title>Kleinheubacher Berichte 2006</volume_title>
		<publication_year>2007</publication_year>
	</journal>
	<doi>10.5194/ars-5-407-2007</doi>
	<article_url>http://www.adv-radio-sci.net/5/407/2007/</article_url>
	<abstract_html>http://www.adv-radio-sci.net/5/407/2007/ars-5-407-2007.html</abstract_html>
	<fulltext_pdf>http://www.adv-radio-sci.net/5/407/2007/ars-5-407-2007.pdf</fulltext_pdf>
	<start_page>407</start_page>
	<end_page>412</end_page>
	<publication_date>2007-06-13</publication_date>
	<article_title content_type="html">LOFAR in Germany</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>W. Reich</name>
			<email>wreich@mpifr-bonn.mpg.de</email>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Max-Planck-Institut für Radioastronomie, Auf dem Hügel  69, 53121 Bonn, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">The LOw Frequency ARray &amp;ndash; LOFAR &amp;ndash; is a new fully digital radio
telescope designed for frequencies between 30 MHz and 240 MHz
centered in the Netherlands. In May 2006 ten German institutes
formed the German LOng Wavelength consortium &amp;ndash; GLOW &amp;ndash; to coordinate
its contributions and scientific interests to the LOFAR project. The
first LOFAR station CS1 was installed in summer 2006 near
Exloo/Netherlands. The second station IS-G1 is presently been placed
in the immediate vicinity of the Effelsberg 100-m radio telescope
near Bad Münstereifel/Germany. This contribution briefly describes
the basic properties and aims of LOFAR, the aims of the GLOW
consortium and the actual activities to install a LOFAR station at
the Effelsberg site.</abstract>
	<references>
		<reference numeration="1" content_type="text"> % vor jede Referenz Beck, R.: Sterne und Weltraum, 9, 22&amp;ndash;33, 2006. </reference>
		<reference numeration="2" content_type="text"> % vor jede Referenz Beck, R. and Reich, W.: Sterne und Weltraum, 9, 19&amp;ndash;21, 2006. </reference>
		<reference numeration="3" content_type="text"> Bregmann, J. D.: in Proc. SPIE Vol. 4015, Radio Telescopes, edited by: Butcher, H. R., 19&amp;ndash;32, 2000. </reference>
		<reference numeration="4" content_type="text"> % vor jede Referenz Brüggen, M., Beck, R., and Falcke, H.: Reviews of Modern Astronomy, 19, 277&amp;ndash;292, 2006. </reference>
		<reference numeration="5" content_type="text"> Falcke, H., van Haarlem, M. P., de Bruyn, A. G. et al.: in: Highlights of Astronomy, 14, XXVth IAU General Assembly, edited by van der Hucht, K. A., 119&amp;ndash;120, 2006. </reference>
	</references>
</article>

