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Sökning: onr:"swepub:oai:research.chalmers.se:340c461c-07f4-4dba-bc83-c2a4b44f8013" > Sub-arcsecond imagi...

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FältnamnIndikatorerMetadata
00013600naa a2201357 4500
001oai:research.chalmers.se:340c461c-07f4-4dba-bc83-c2a4b44f8013
003SwePub
008220212s2022 | |||||||||||000 ||eng|
009oai:DiVA.org:su-202432
024a https://doi.org/10.1051/0004-6361/2021406492 DOI
024a https://research.chalmers.se/publication/5286502 URI
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-2024322 URI
040 a (SwePub)cthd (SwePub)su
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Morabito, L.u Durham University4 aut
2451 0a Sub-arcsecond imaging with the International LOFAR Telescope: I. Foundational calibration strategy and pipeline
264 c 2022-01-25
264 1b EDP Sciences,c 2022
338 a electronic2 rdacarrier
520 a The International LOFAR Telescope is an interferometer with stations spread across Europe. With baselines of up to ∼2000 km, LOFAR has the unique capability of achieving sub-arcsecond resolution at frequencies below 200 MHz. However, it is technically and logistically challenging to process LOFAR data at this resolution. To date only a handful of publications have exploited this capability. Here we present a calibration strategy that builds on previous high-resolution work with LOFAR. It is implemented in a pipeline using mostly dedicated LOFAR software tools and the same processing framework as the LOFAR Two-metre Sky Survey (LoTSS). We give an overview of the calibration strategy and discuss the special challenges inherent to enacting high-resolution imaging with LOFAR, and describe the pipeline, which is publicly available, in detail. We demonstrate the calibration strategy by using the pipeline on P205+55, a typical LoTSS pointing with an 8 h observation and 13 international stations. We perform in-field delay calibration, solution referencing to other calibrators in the field, self-calibration of these calibrators, and imaging of example directions of interest in the field. We find that for this specific field and these ionospheric conditions, dispersive delay solutions can be transferred between calibrators up to ∼1.5° away, while phase solution transferral works well over ∼1°. We also demonstrate a check of the astrometry and flux density scale with the in-field delay calibrator source. Imaging in 17 directions, we find the restoring beam is typically ∼0.3″ ×0.2″ although this varies slightly over the entire 5 deg2 field of view. We find we can achieve ∼80-300 μJy bm-1 image rms noise, which is dependent on the distance from the phase centre; typical values are ∼90 μJy bm-1 for the 8 h observation with 48 MHz of bandwidth. Seventy percent of processed sources are detected, and from this we estimate that we should be able to image roughly 900 sources per LoTSS pointing. This equates to ∼ 3 million sources in the northern sky, which LoTSS will entirely cover in the next several years. Future optimisation of the calibration strategy for efficient post-processing of LoTSS at high resolution makes this estimate a lower limit.
650 7a NATURVETENSKAPx Fysikx Annan fysik0 (SwePub)103992 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Other Physics Topics0 (SwePub)103992 hsv//eng
650 7a TEKNIK OCH TEKNOLOGIERx Elektroteknik och elektronikx Signalbehandling0 (SwePub)202052 hsv//swe
650 7a ENGINEERING AND TECHNOLOGYx Electrical Engineering, Electronic Engineering, Information Engineeringx Signal Processing0 (SwePub)202052 hsv//eng
650 7a NATURVETENSKAPx Data- och informationsvetenskapx Datorseende och robotik0 (SwePub)102072 hsv//swe
650 7a NATURAL SCIENCESx Computer and Information Sciencesx Computer Vision and Robotics0 (SwePub)102072 hsv//eng
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a Galaxies: jets
653 a Galaxies: active
653 a Radiation mechanisms: non-thermal
653 a Techniques: high angular resolution
700a Jackson, N. J.u University of Manchester4 aut
700a Mooney, S.u Jagiellonian University in Kraków, Poland4 aut
700a Sweijen, F.u Universiteit Leiden (UL),Leiden University (UL)4 aut
700a Badole, S.u University of Manchester4 aut
700a Kukreti, P.u Netherlands Institute for Radio Astronomy (ASTRON),Rijksuniversiteit Groningen,University of Groningen4 aut
700a Venkattu, Deepikau Stockholms universitet,Institutionen för astronomi,Alba Nova Universitetscentrum,AlbaNova University Center. Stockholm Center for Physics, Astronomy and Biotechnology4 aut0 (Swepub:su)deve3138
700a Groeneveld, C.u Universiteit Leiden (UL),Leiden University (UL)4 aut
700a Kappes, A.u Julius-Maximilians Universität Würzburg,University of Würzburg4 aut
700a Bonnassieux, E.u Universita di Bologna,University of Bologna4 aut
700a Drabent, A.u Thüringer Landessternwarte Tautenburg4 aut
700a Iacobelli, M.u Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a Croston, J. H.u Open University4 aut
700a Best, P. N.u University of Edinburgh4 aut
700a Bondi, M.u Istituto di Radioastronomia4 aut
700a Callingham, J. R.u Netherlands Institute for Radio Astronomy (ASTRON),Universiteit Leiden (UL),Leiden University (UL)4 aut
700a Conway, John,d 1963u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)jconway
700a Deller, A.u Swinburne University of Technology,Deutsches Elektronen-Synchrotron (DESY),Friedrich-Alexander-Universität Erlangen Nurnberg (FAU)4 aut
700a Hardcastle, M. J.u University of Hertfordshire,Netherlands Institute for Radio Astronomy (ASTRON),Rijksuniversiteit Groningen,University of Groningen,Instituto de Astrofisica de Andalucía (IAA),Institute of Astrophysics of Andalusia (IAA)4 aut
700a McKean, J.u Netherlands Institute for Radio Astronomy (ASTRON),Rijksuniversiteit Groningen,University of Groningen,Deutsches GeoForschungsZentrum (GFZ),German Research Centre for Geosciences (GFZ),Technische Universität Berlin,Technische Universiteit Eindhoven,Eindhoven University of Technology,Station de Radioastronomie de Nançay,Universite d'Orleans,University of Orléans4 aut
700a Miley, G. K.u Universiteit Leiden (UL),Leiden University (UL),Julius-Maximilians Universität Würzburg,University of Würzburg4 aut
700a Moldon, J.u Instituto de Astrofisica de Andalucía (IAA),Institute of Astrophysics of Andalusia (IAA)4 aut
700a Röttgering, H. J.A.u Universiteit Leiden (UL),Leiden University (UL),Shell Technology Center,Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a Tasse, C.u Observatoire de Paris-Meudon,Rhodes University4 aut
700a Shimwell, T. W.u Netherlands Institute for Radio Astronomy (ASTRON),Universiteit Leiden (UL),Leiden University (UL)4 aut
700a van Weeren, R.u Universiteit Leiden (UL),Leiden University (UL),Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut
700a Anderson, J. M.u Deutsches GeoForschungsZentrum (GFZ),German Research Centre for Geosciences (GFZ),Technische Universität Berlin4 aut
700a Asgekar, A.u Shell Technology Center,Netherlands Institute for Radio Astronomy (ASTRON),Universita di Bologna,University of Bologna,Istituto di Radioastronomia,Universität Hamburg,University of Hamburg,Vrije Universiteit Brüssel (VUB),Vrije Universiteit Brussel (VUB),Radboud Universiteit,Radboud University,University of Manchester,Universiteit Leiden (UL),Leiden University (UL),George Washington University,University of Warmia and Mazury in Olsztyn,Universiteit Van Amsterdam,University of Amsterdam4 aut
700a Avruch, I.M.u Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a van Bemmel, I.u Joint Institute for VLBI in Europe (JIVE)4 aut
700a Bentum, M. J.u Technische Universiteit Eindhoven,Eindhoven University of Technology,Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a Bonafede, A.u Universita di Bologna,University of Bologna,Istituto di Radioastronomia,Universität Hamburg,University of Hamburg4 aut
700a Brouw, W. N.u Rijksuniversiteit Groningen,University of Groningen4 aut
700a Butcher, H. R.u Australian National University,Polish Academy of Sciences4 aut
700a Ciardi, B.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut
700a Corstanje, A.u Vrije Universiteit Brüssel (VUB),Vrije Universiteit Brussel (VUB),Radboud Universiteit,Radboud University4 aut
700a Coolen, A. H.W.M.u Netherlands Institute for Radio Astronomy (ASTRON),Thüringer Landessternwarte Tautenburg4 aut
700a Damstra, Siedsu Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a De Gasperin, F.u Universität Hamburg,University of Hamburg,Istituto di Radioastronomia4 aut
700a Duscha, S.u Netherlands Institute for Radio Astronomy (ASTRON),Universität Bielefeld,Bielefeld University4 aut
700a Eisloffel, J.u Thüringer Landessternwarte Tautenburg,Ruhr-Universität Bochum4 aut
700a Engels, D.u Universität Hamburg,University of Hamburg4 aut
700a Falcke, H.D.u Radboud Universiteit,Radboud University4 aut
700a Garrett, M. A.u University of Manchester,Universiteit Leiden (UL),Leiden University (UL),Leibniz-Institut Für Astrophysik Potsdam,Leibniz Institute for Astrophysics Potsdam4 aut
700a Grießmeier, J.M.u Station de Radioastronomie de Nançay,Universite d'Orleans,University of Orléans4 aut
700a Gunst, A.W.u Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a van Haarlem, M. P.u Netherlands Institute for Radio Astronomy (ASTRON),Rijksuniversiteit Groningen,University of Groningen,Université de Lyon4 aut
700a Hoeft, M.u Thüringer Landessternwarte Tautenburg4 aut
700a van der Horst, A. J.u George Washington University4 aut
700a Jutte, E.u Ruhr-Universität Bochum4 aut
700a Kadler, M.u Julius-Maximilians Universität Würzburg,University of Würzburg4 aut
700a Koopmans, L.V.E.u Rijksuniversiteit Groningen,University of Groningen4 aut
700a Krankowski, A.u University of Warmia and Mazury in Olsztyn4 aut
700a Mann, G.u Leibniz-Institut Für Astrophysik Potsdam,Leibniz Institute for Astrophysics Potsdam4 aut
700a Nelles, A.u Deutsches Elektronen-Synchrotron (DESY),Friedrich-Alexander-Universität Erlangen Nurnberg (FAU)4 aut
700a Oonk, J. B. R.u Surfsara Bv4 aut
700a Orrú, E.u Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a Paas, H.u Rijksuniversiteit Groningen,University of Groningen4 aut
700a Pandey, V. N.u Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a Pizzo, R.u Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a Pandey-Pommier, M.u Université de Lyon,LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique,Station de Radioastronomie de Nançay4 aut
700a Reich, W.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut
700a Rothkaehl, Hannau Polish Academy of Sciences4 aut
700a Ruiter, Marku Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a Schwarz, D. J.u Universität Bielefeld,Bielefeld University4 aut
700a Shulevski, A.u Universiteit Van Amsterdam,University of Amsterdam,Universiteit Leiden (UL),Leiden University (UL)4 aut
700a Soida, M.u Jagiellonian University in Kraków, Poland4 aut
700a Tagger, M.u Universite d'Orleans,University of Orléans4 aut
700a Vocks, C.u Leibniz-Institut Für Astrophysik Potsdam,Leibniz Institute for Astrophysics Potsdam4 aut
700a Wijers, Ramju Universiteit Van Amsterdam,University of Amsterdam4 aut
700a Wijnholds, S. J.u Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a Wucknitz, O.u Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)4 aut
700a Zarka, P.M.u LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique,Station de Radioastronomie de Nançay4 aut
700a Zucca, P.u Netherlands Institute for Radio Astronomy (ASTRON)4 aut
710a Durham Universityb University of Manchester4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 658q 658x 0004-6361x 1432-0746
856u https://research.chalmers.se/publication/528650/file/528650_Fulltext.pdfx primaryx freey FULLTEXT
856u https://www.aanda.org/articles/aa/pdf/forth/aa40649-21.pdf
856u https://doi.org/10.1051/0004-6361/202140649y Fulltext
8564 8u https://doi.org/10.1051/0004-6361/202140649
8564 8u https://research.chalmers.se/publication/528650
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-202432

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