Abstract
Original language | English |
---|---|
Article number | A2 |
Number of pages | 53 |
Journal | Astronomy & Astrophysics |
Volume | 556 |
DOIs | |
Publication status | Published - 2013 |
Externally published | Yes |
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In: Astronomy & Astrophysics, Vol. 556, A2, 2013.
Research output: Contribution to journal › Article › Research › peer-review
TY - JOUR
T1 - LOFAR
T2 - the LOw-frequency ARray
AU - van Haarlem, Michael P
AU - Wise, Michael W
AU - Gunst, Andre
AU - Heald, George
AU - McKean, John P
AU - Hessels, Jason W T
AU - de Bruyn, A Ger
AU - Nijboer, Ronald
AU - Swinbank, John D
AU - Fallows, Richard A
AU - Brentjens, Michiel A
AU - Nelles, Anna
AU - Beck, Rainer
AU - Falcke, Heino
AU - Fender, Rob
AU - Horandel, Jorg R
AU - Koopmans, Leon V E
AU - Mann, Gottfried
AU - Miley, George K
AU - Rottgering, Huub J A
AU - Stappers, Benjamin W
AU - Wijers, Ralph A M J
AU - Zaroubi, Saleem
AU - van den Akker, Martin
AU - Alexov, Anastasia
AU - Anderson, James M
AU - Anderson, Kenneth R
AU - van Ardenne, Arnold
AU - Arts, Michel J
AU - Asgekar, Ashish
AU - Avruch, Ian M
AU - Batejat, Fabien
AU - Bahren, Lars
AU - Bell, Martin E
AU - Bell, Michael R
AU - van Bemmel, Ilse
AU - Bennema, Peter
AU - Bentum, Mark J
AU - Bernardi, Gianni
AU - Best, Philip N
AU - Birzan, Laura
AU - Bonafede, Annalisa
AU - Boonstra, Albert-Jan
AU - Braun, Robert
AU - Bregman, Jaap D
AU - Breitling, Frank
AU - van den Brink, Raymond H
AU - Broderick, Jess W
AU - Broekema, P Chris
AU - Brouw, Wim N
AU - Bruggen, Marcus
AU - Butcher, Harvey Raymond
AU - van Cappellen, Wim A
AU - Ciardi, Benedetta
AU - Coenen, Thijs
AU - Conway, John E
AU - Coolen, Arthur
AU - Corstanje, Arthur
AU - Damstra, Sieds
AU - Davies, O
AU - Deller, Adam Travis
AU - Dettmar, Ralf-Jurgen
AU - van Diepen, Ger
AU - Dijkstra, Klass
AU - Donker, Pieter
AU - Doorduin, Arie
AU - Dromer, J
AU - Drost, Marco
AU - van Duin, Albert
AU - Eisloffel, Jochen
AU - van Enst, Joris
AU - Ferrari, Chiara
AU - Frieswijk, Wilfred
AU - Gankema, J A Hans
AU - Garrett, Michael A
AU - de Gasperin, Francesco
AU - Gerbers, Marchel
AU - de Geus, Eugene J
AU - Griessmeier, Jean-Mathias
AU - Grit, Tuen
AU - Gruppen, Peter
AU - Hamaker, Johan
AU - Hassall, Tom E
AU - Hoeft, Matthias
AU - Holties, Hanno A
AU - Horneffer, Andreas
AU - van der Horst, Alexander J
AU - van Houwelingen, Andre
AU - Huijgen, Arie
AU - Iacobelli, Marco
AU - Intema, Huib T
AU - Jackson, Neal J
AU - Jelic, Vibor
AU - de Jong, Alwin
AU - Jutte, Eva
AU - Kant, G W Dion
AU - Karastergiou, Aris
AU - Koers, H U A Arjen
AU - Kollen, Hans
AU - Kondratiev, Vlad I
AU - Kooistra, Eric
AU - Koopman, Yde J
AU - Koster, Anne
AU - Kuniyoshi, Masaya
AU - Kramer, Michael
AU - Kuper, Geert
AU - Lambropoulos, Peter Panagiotis
AU - Law, Casey J
AU - van Leeuwen, Joeri
AU - Lemaitre, Jerome
AU - Loose, Marcel
AU - Maat, Peter
AU - Macario, Giulia
AU - Markoff, Sera B
AU - Masters, Joseph S
AU - McFadden, Rebecca A
AU - McKay-Bukowski, Derek
AU - Meijering, Hopko
AU - Meulman, Henri
AU - Mevius, Maaijke
AU - Middelberg, Enno
AU - Millenaar, Rob
AU - Miller-Jones, James C A
AU - Mohan, Niruj Ramanujam
AU - Mol, Jan David
AU - Morawietz, Juergen
AU - Morganti, Raffaella
AU - Mulcahy, David Declan
AU - Mulder, Eim
AU - Munk, Harm
AU - Nieuwenhuis, Lambert
AU - van Nieuwpoort, Rob V
AU - Noordam, Jan E
AU - Norden, Menno
AU - Noutsos, Aris
AU - Offringa, Andre R
AU - Olofsson, Hans
AU - Omar, Amitesh
AU - Orru, Emanuela
AU - Overeem, Ruud
AU - Paas, Harm
AU - Pommier, Mamta
AU - Pandey, Vishambar N
AU - Pizzo, Roberto
AU - Polatidis, Antonis
AU - Rafferty, David A
AU - Rawlings, Steven
AU - Reich, Wolfgang
AU - de Reijer, Jan-Pieter
AU - Reitsma, Jan
AU - Renting, G Adriaan
AU - Riemers, Paul
AU - Rol, Evert
AU - Romein, John W
AU - Roosjen, Jan
AU - Ruiter, Mark
AU - Scaife, Anna
AU - van der Schaaf, Kjeld
AU - Scheers, Bart
AU - Schellart, Pim
AU - Schoenmakers, Arno
AU - Schoonderbeek, Gijs
AU - Serylak, Maciej
AU - Shulevski, Alexander
AU - Sluman, Jurjen
AU - Smirnov, Oleg
AU - Sobey, Charlotte
AU - Spreeuw, Hanno
AU - Steinmetz, Matthias
AU - Sterks, Cees G M
AU - Stiepel, Harm Jan
AU - Stuurwold, Klaas
AU - Tagger, Michel
AU - Tang, Yuan
AU - Tasse, Cyril
AU - Thomas, Ivan
AU - Thoudam, Satyendra
AU - Toribio, Maria Carmen
AU - van der Tol, Bas
AU - Usov, Oleksander
AU - van Veelen, Martijn
AU - van der Veen, Alle-Jan
AU - ter Veen, Sander
AU - Verbiest, Joris P W
AU - Vermeulen, Rene
AU - Vermaas, Nico
AU - Vocks, Christian
AU - Vogt, Corina
AU - de Vos, Marco
AU - van der Wal, Erik
AU - van Weeren, Reinout
AU - Weggemans, Hans
AU - Weltevrede, Patrick
AU - White, Simon D M
AU - Wijnholds, Stefan J
AU - Wilhelmsson, Tomas
AU - Wucknitz, Olaf
AU - Yatawatta, Sarod
AU - Zarka, Philippe
AU - Zensus, J Anton
AU - van Zwieten, Joris E
PY - 2013
Y1 - 2013
N2 - LOFAR, the LOw-Frequency ARray, is a new-generation radio interferometer constructed in the north of the Netherlands and across europe. Utilizing a novel phased-array design, LOFAR covers the largely unexplored low-frequency range from 10-240 MHz and provides a number of unique observing capabilities. Spreading out from a core located near the village of Exloo in the northeast of Netherlands, a total of 40 LOFAR stations are nearing completion. A further five stations have been deployed throughout Germany, and one station has been built in each of France, Sweden, and the UK. Digital beam-forming techniques make the LOFAR system agile and allow for rapid repointing of the telescope as well as the potential for multiple simultaneous observations. With its dense core array and long interferometric baselines, LOFAR achieves unparalleled sensitivity and angular resolution in the low-frequency radio regime. The LOFAR facilities are jointly operated by the International LOFAR Telescope (ILT) foundation, as an observatory open to the global astronomical community. LOFAR is one of the first radio observatories to feature automated processing pipelines to deliver fully calibrated science products to its user community. LOFAR s new capabilities, techniques and modus operandi make it an important pathfinder for the Square Kilometre Array (SKA). We give an overview of the LOFAR instrument, its major and software components, and the core science objectives that have driven its design. In addition, we present a selection of new results from the commissioning phase of this new radio observatory.
AB - LOFAR, the LOw-Frequency ARray, is a new-generation radio interferometer constructed in the north of the Netherlands and across europe. Utilizing a novel phased-array design, LOFAR covers the largely unexplored low-frequency range from 10-240 MHz and provides a number of unique observing capabilities. Spreading out from a core located near the village of Exloo in the northeast of Netherlands, a total of 40 LOFAR stations are nearing completion. A further five stations have been deployed throughout Germany, and one station has been built in each of France, Sweden, and the UK. Digital beam-forming techniques make the LOFAR system agile and allow for rapid repointing of the telescope as well as the potential for multiple simultaneous observations. With its dense core array and long interferometric baselines, LOFAR achieves unparalleled sensitivity and angular resolution in the low-frequency radio regime. The LOFAR facilities are jointly operated by the International LOFAR Telescope (ILT) foundation, as an observatory open to the global astronomical community. LOFAR is one of the first radio observatories to feature automated processing pipelines to deliver fully calibrated science products to its user community. LOFAR s new capabilities, techniques and modus operandi make it an important pathfinder for the Square Kilometre Array (SKA). We give an overview of the LOFAR instrument, its major and software components, and the core science objectives that have driven its design. In addition, we present a selection of new results from the commissioning phase of this new radio observatory.
U2 - 10.1051/0004-6361/201220873
DO - 10.1051/0004-6361/201220873
M3 - Article
SN - 0004-6361
VL - 556
JO - Astronomy & Astrophysics
JF - Astronomy & Astrophysics
M1 - A2
ER -