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	DBLP: Wolfgang Effelsberg
		Claudia Schremmer, Volker Hilt, Wolfgang Effelsberg: Erfahrungen mit synchronen und asynchronen Lernszenarien an der Universität Mannheim.
		Wolfgang Effelsberg: Erfahrungen aus den TeleTeaching-Projekten der Universität Mannheim.
		Wolfgang Effelsberg, Hans Werner Meuer, Günter Müller: Kommunikation in Verteilten Systemen, Grundlagen, Anwendungen, Betrieb, GI/ITG-Fachtagung, Mannheim, 20.-22.
	www.informatik.uni-trier.de /~ley/db/indices/a-tree/e/Effelsberg:Wolfgang.html (1574 words)

	[No title]
		Effelsberg has station name 'EB_VLBA' Arecibo has station name 'ARECIBO' GBT has station name 'GBT_VLBA' The phased VLA has station name 'VLA27' The SCHED manual can be read on the WWW at: http://www.aoc.nrao.edu/~cwalker/sched/sched/sched.html 3) Arecibo and Effelsberg do not support automatic tape allocation.
		Furthermore, Effelsberg has only 1 recorder, so an observing gap of 10 minutes is necessary to allow for tape changes (see the HSA at EB document at http://www.mpifr-bonn.mpg.de/EVN/HSA-EB for more information).
		Be aware that if the last tape pass is not recorded continuously, but involves intermediate stopping of the tape, then a feature of the NRAO scheduling software executes a "post-pass" forward and reverse winding of the tape.
	www.nrao.edu /HSA/HSA-Tips.txt (680 words)

	2nd quadrant Galactic SNRs
		Effelsberg 100-m at 4.85 (2'.4), 8.35 (1'.4), 10.5 (1'.2) and 32 GHz (0'.45) of pulsar wind nebula, including polarisation.
		WSRT and Effelsberg 100-m at 1.4 GHz (50"), and VLA at 1.4 GHz (13"), for neutral hydrogen studies.
		Effelsberg 100-m at 1.4 (9'.4), 2.7 (4'.3) and 4.75 GHz (2'.4).
	www.mrao.cam.ac.uk /surveys/snrs/snrs.2nd.html (1444 words)

	NRAO: High Sensitivity Array
		By adding the GBT, phased VLA, Arecibo, and Effelsberg to a VLBA experiment the sensitivity can be increased by an order of magnitude (see figure at left showing sensitivities for a 1 hour integration recording at 256 Mbps).
		Effelsberg has often been used in conjunction with the VLBA, and is frequency agile at 5 GHz and above.
		For more information about including Effelsberg with the HSA consult these notes by Richard Porcas.
	www.nrao.edu /HSA (247 words)

	PI4 - Publications
		Ralf Schmitz, Marc Torrent-Moreno, Hannes Hartenstein, Wolfgang Effelsberg
		Gerald Kühne, Joachim Weickert, Markus Beier, Wolfgang Effelsberg
		Claudia Schremmer, Wolfgang Effelsberg, Jean-Claude Grattarola, Edoardo Berera
	www.informatik.uni-mannheim.de /pi4/publications/effelsberg (3525 words)

	porcas1
		This report lists a number of developments at the Effelsberg 100m telescope since the last Working Group meeting which may be of relevance for geodetic VLBI observing.
		Bug fixes and new facilities such as barrel roll were successfully tested in a geodetic VLBI experiment correlated in Bonn.
		Work continues on both the water vapour radiometer and the plans for installing a GPS receiver in Effelsberg, for providing auxiliary phase and delay measurements for VLBI.
	www.ieec.fcr.es /hosted/15wmevga/proceedings/porcas1/porcas1.html (293 words)

	Max Planck Institute for Radio Astronomy, Bonn - Radio Telescope Effelsberg
		With a diameter of 100 meters, the Radio Telescope Effelsberg is one of the largest fully steerable radio telescopes on earth.
		The telescope is employed to observe pulsars, cold gas- and dust clusters, the sites of star formation, jets of matter emitted by fl holes and the nuclei (centres) of distant far-off galaxies.
		Effelsberg is an important part of the worldwide network of radio telescopes.
	www.mpifr.de /english/radiotelescope/index.html (139 words)

	GRB030329 (Site not responding. Last check: 2007-10-28)
		After 4 days the standard fireball models predict a size for the afterglow of just 10e17 cm or 0.01 mas, but still large enough to begin quenching the scintillation as confirmed in the second VLBI epoch 7 days after the burst.
		A third VLBI epoch including Effelsberg and going to 22 GHz to maximize resolution measured the size of the afterglow to be 0.08 mas 24 days after the burst.
		The observing frequency was again 8.4 GHz, and the size predicted by the standard fireball model was 0.2 mas.
	www.naic.edu /~astro/aovlbi/GRB030329/GRB030329.html (555 words)

	[No title]
		Matthias Transier, Holger Füßler, Jörg Widmer, Martin Mauve, Wolfgang Effelsberg.
		Martin Mauve, Hannes Hartenstein, Holger Füßler, Jörg Widmer, Wolfgang Effelsberg.
		Jürgen Vogel, Jörg Widmer, Dirk Farin, Martin Mauve, Wolfgang Effelsberg.
	www.cn.uni-duesseldorf.de /publications/details/mauve.html (1826 words)

	L-Band Wide Observations (Site not responding. Last check: 2007-10-28)
		The Effelsberg Mid-latitude survey image of polarised intensity in the same area is shown below the Arecibo image.
		Therefore there is an arbitrary rotation of the polarisation position angle difference between the Effelsberg and Arecibo images.
		However, the polarisation features in the Effelsberg image are seen in the L-band wide data with higher angular resolution, showing, for instance the structure of the dark lanes surrounding the strong source near the centre of the image.
	www.ras.ucalgary.ca /GALFACTS/L-Band_Wide_Observations.html (418 words)

	Germany Wins… « Google Sightseeing
		Arecibo is much larger, but Effelsberg is fully movable while Arecibo is just built into the ground.
		Iirc Effelsberg is the second largest in the world of its kind and indeed it looks pretty impressive.
		Effelsberg is the largest moveable radio telescope in the world, the one in Puerto Rico is the largest non-moveable radio telescope.
	googlesightseeing.com /2006/06/09/germany-wins (675 words)

	:: LOFAR - General Information
		At the end of October 2005, the Max-Planck-Society granted funding for a LOFAR antenna station in Effelsberg (the radio observatory of the Max-Planck-Institut für Radioastronomie (MPIfR) in Bonn).
		Together with an earlier pledge to provide a wide band data transport link to the observatory, the expansion of the LOFAR network outside the Netherlands is becoming reality.
		A plan for a total twelve LOFAR stations at sites in Germany - of which six are planned in more detail already - met an enthusiastic response at the annual autumn meeting of the Astronomische Gesellschaft in Cologne at the end of September 2005.
	www.lofar.org /p/news/Jan06.htm (240 words)

	Pulsar Research at Berkeley
		This system was installed at Effelsberg 100m telescope in 1996 October.
		The signal paths for the coherent and incoherent processors are identical down to the final board.
		Arecibo and Effelsberg have both coherent and incoherent capability while an incoherent system for Green Bank is nearing completion.
	astro.berkeley.edu /~mpulsar/bpp/bpp.shtml (1428 words)

	The Effelsberg 6 cm Survey of the Galactic plane
		A survey of the galactic plane has been made with the Effelsberg 100-m telescope at a frequency of 4.875 GHz with a beamwidth of 2.6'.
		The data are presented as radio contour maps covering l=357.5 to 60^o, b=+-1^o, together a list of 1186 radio sources.
		We therefore did not de-convolve the apparent diameters, or estimate integrated fluxes for the sources.
	cats.sao.ru /doc/6CMBONN.html (471 words)

	The Effelsberg 21 cm Survey (Site not responding. Last check: 2007-10-28)
		We present the results of a radio continuum survey at 21 cm wavelength or the GAlactic plane between 357
		The Effelsberg 21 cm radio comtinuum survey of the Galactic plane between l=95.5d and 240d
		We present the results of a radio continuum survey at 21 cm wavelength orthe Galactic plane between 95.5 < l < 240 and -4 < l < +5o with the Effelsberg 100-m radio telescope.
	cats.sao.ru /doc/21CMBONN.html (294 words)

	[No title]
		Relevant deadlines are also mentioned, as are how to use the vlbiobs account at the Array Operations Center (AOC) and how to monitor the VLBA's actions during your program.
		Effelsberg has only 1 tape drive, so automatic tape allocation is not practical; for that station you must allow a tape change gap of 10-15 minutes and follow the tape management advice in The Sched User Manual (see section 5) concerning tape usage and postpass avoidance.
		The phased VLA has special calibration needs; you can ensure that these needs are met if you use the scheduling program sched (see section 5) to make your VLA schedule files.
	www.vlba.nrao.edu /astro/obsprep/before/before.if.txt (935 words)

	Radio Observations of the Great Comet Crash
		When it became obvious that comet P/Shoemaker-Levy 9 would impact Jupiter in July 1994 the Effelsberg 100 m radio telescope of the Max-Planck-Institut für Radioastronomie became a key link in a world-wide network of radio telescopes to monitor this unique event.
		Full polarization measurements of the Jovian radio emission were performed at Effelsberg before, during and after the impacts at three different wavelengths (frequencies): 2.8 cm (10.55 GHz), 6.3 cm (4.75 GHz) and 11.1 cm (2.695 GHz).
		In Figure 3 the evaluation of the nonthermal flux density during the whole impact week is shown for 11 cm and 6 cm wavelength as a function of universal time UT. The times of impacts during the Effelsberg view periods are marked with a vertical arrow and the corresponding name of the fragment.
	www.astro.uni-bonn.de /~mbird/SL9/doc_fr.html (3363 words)

	LOFAR:UK uv simulations and point source response
		Dutch core + Effelsberg, Garching, Potsdam, Jodrell, Cambridge(ps.gz)
		Dutch core + Effelsberg, Garching, Potsdam, Jodrell, Cambridge, Chilbolton(ps.gz)
		Dutch core + Effelsberg, Garching, Potsdam, Jodrell, Cambridge, Chilbolton, Edinburgh(ps.gz)
	www.jb.man.ac.uk /~rbeswick/LOFAR (598 words)

	Panoramic View of the Effelsberg 100-m Telescope
		A panoramic view of the Effelsberg 100-m radio telescope of the Max-Planck-Institute for Radio Astronomy in Bonn, Germany.
		The picture has been stitched from six single photographs taken with a Canon D-30 digital SLR camera through a Canon EF 20/2.8 wide angle lens.
		The valley on the right allows the telescope to observe the galactic centre for a few hours each day.
	www.atnf.csiro.au /people/Enno.Middelberg/effelsberg-pano/effelsberg-pano.html (62 words)

	Mr Peck's views the stars through a very long lens
		Dad and Alison posing for a countryside photo in the Effelsberg region of Germany, with the sneaky radio telescope, like Ashcroft, watching over them.
		Following all which, Marlowe and her Papa returned to Switzerland for some rainy hiking, and months later Alison came down to hike about a bit as well.
		Visit to Alison at the Effelsberg radio telescope in Germany
	www.dpeck.info /vac/vac2001d.htm (413 words)

	DBLP: Jürgen Vogel
		Jürgen Vogel, Werner Geyer, Li-Te Cheng, Michael J. Muller: Consistency Control for Synchronous and Asynchronous Collaboration Based on Shared Objects and Activities.
		Volker Hilt, Martin Mauve, Jürgen Vogel, Wolfgang Effelsberg: Interactive media on demand: generic recording and replay of interactive media streams.
		Rüdiger Weis, Jürgen Vogel, Wolfgang Effelsberg, Werner Geyer, Stefan Lucks: How to Make a Digital Whiteboard Secure - Using Java-Cards for Multimedia Applications.
	www.vldb.org /dblp/db/indices/a-tree/v/Vogel:J=uuml=rgen.html (291 words)

	Effelsberg
		3 x Weitkulturerbe, Beethoven-, Schumann-, Adenauerhaus, Posttower, Bundeshaus, Nürburgring und Effelsberg das größte Radioteleskop der Welt – Sensationen im Rheinland...
		Durch einen Arbeitkollegen hatte ich die Gelegenheit mir das Radioteleskop in Effelsberg (Eifel) aus nächster Nähe ansehen zu können.
		Ein Freund von ihm ist dort als Wissenschaftler tätig und für die Positionierung verantwortlich.
	www.die-region.info /behinderten/effelsberg.php (212 words)

	Publications
		Silvia Pfeiffer, Rainer Lienhart, Stephan Fischer and Wolfgang Effelsberg, Abstracting Digital Movies Automatically, Journal of Visual Communication and Image Representation, Vol.
		Silvia Pfeiffer, Rainer Lienhart, Gerald Kühne and Wolfgang Effelsberg.
		Rainer Lienhart, Silvia Pfeiffer and Wolfgang Effelsberg, The MoCA Workbench: Support for Creativity in Movie Content Analysis, Proc.
	www.lienhart.de /Publications/publications.html (1005 words)

	Radioteleskop Effelsberg pictures from scenery & nature photos on webshots
		Radioteleskop Effelsberg pictures from scenery and nature photos on webshots
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	outdoors.webshots.com /photo/1206593376047057079iwVScY (138 words)

	LinkedIn: Wolfgang Effelsberg
		See who you and Wolfgang Effelsberg know in common
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	www.linkedin.com /pub/0/634/406 (61 words)

	Pat Cotter Genealogy
		including Effelsberg, Lethert, Tondorf, Esch, Mutscheid, Scheuerheck- and any other close towns!
		Pat Cotter - researching Lethert, Mahlberg, Fussel, Linden - in towns of Esch, Lethert, Effelsberg
		Mark Honerd - ancestors from Effelsberg/Lethert include Honert
	www.rootsweb.com /~cotter/Effelsberg.htm (76 words)

	dnb, Impressum
		Kathrin Ansorge, Hannelore Effelsberg, Marcus Klein, Britta Meister, Michaela Michel, Monika Pfitzner, Thomas Seidel, Silke Sewing, Roberto Vásquez
		Allgemeine Anfragen im Zusammenhang mit dem Informations-Server der Deutschen Nationalbibliothek beantwortet die Redaktion.
		Von diesen eigenen Inhalten sind Querverweise ("Links") auf die von anderen Anbietern bereitgehaltenen Inhalte zu unterscheiden, für die die Deutsche Nationalbibliothek keinerlei Haftung übernimmt.
	www.ddb.de /impressum (107 words)

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