Sub-arcsecond imaging with the International LOFAR Telescope: I. Foundational calibration strategy and pipeline
Artikel i vetenskaplig tidskrift, 2022
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.
Galaxies: jets
Galaxies: active
Radiation mechanisms: non-thermal
Techniques: high angular resolution
Författare
L. Morabito
Durham University
N. J. Jackson
University of Manchester
S. Mooney
University College Dublin
F. Sweijen
Universiteit Leiden
S. Badole
University of Manchester
P. Kukreti
Netherlands Institute for Radio Astronomy (ASTRON)
Rijksuniversiteit Groningen
D. Venkattu
Alba Nova Universitetscentrum
C. Groeneveld
Universiteit Leiden
A. Kappes
Julius-Maximilians Universität Würzburg
E. Bonnassieux
Universita di Bologna
A. Drabent
Thüringer Landessternwarte Tautenburg
M. Iacobelli
Netherlands Institute for Radio Astronomy (ASTRON)
J. H. Croston
Open University
P. N. Best
University of Edinburgh
M. Bondi
Istituto di Radioastronomia
J. R. Callingham
Netherlands Institute for Radio Astronomy (ASTRON)
Universiteit Leiden
John Conway
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
A. Deller
Swinburne University of Technology
M. J. Hardcastle
University of Hertfordshire
J. McKean
Netherlands Institute for Radio Astronomy (ASTRON)
Rijksuniversiteit Groningen
G. K. Miley
Universiteit Leiden
J. Moldon
Instituto de Astrofisica de Andalucía (IAA)
H. J.A. Röttgering
Universiteit Leiden
C. Tasse
Observatoire de Paris-Meudon
Rhodes University
T. W. Shimwell
Netherlands Institute for Radio Astronomy (ASTRON)
Universiteit Leiden
R. van Weeren
Universiteit Leiden
J. M. Anderson
Deutsches GeoForschungsZentrum (GFZ)
Technische Universität Berlin
A. Asgekar
Shell Technology Center
Netherlands Institute for Radio Astronomy (ASTRON)
I.M. Avruch
Sci & Technol BV
Netherlands Institute for Radio Astronomy (ASTRON)
I. van Bemmel
Joint Institute for VLBI in Europe (JIVE)
M. J. Bentum
Technische Universiteit Eindhoven
Netherlands Institute for Radio Astronomy (ASTRON)
A. Bonafede
Universita di Bologna
Istituto di Radioastronomia
Universität Hamburg
W. N. Brouw
Rijksuniversiteit Groningen
H. R. Butcher
Australian National University
B. Ciardi
Max-Planck-Gesellschaft
A. Corstanje
Vrije Universiteit Brüssel (VUB)
Radboud Universiteit
A. H.W.M. Coolen
Netherlands Institute for Radio Astronomy (ASTRON)
Sieds Damstra
Netherlands Institute for Radio Astronomy (ASTRON)
F. De Gasperin
Universität Hamburg
Istituto di Radioastronomia
S. Duscha
Netherlands Institute for Radio Astronomy (ASTRON)
J. Eisloffel
Thüringer Landessternwarte Tautenburg
D. Engels
Universität Hamburg
H.D. Falcke
Radboud Universiteit
M. A. Garrett
University of Manchester
Universiteit Leiden
J.M. Grießmeier
Station de Radioastronomie de Nançay
Universite d'Orleans
A.W. Gunst
Netherlands Institute for Radio Astronomy (ASTRON)
M. P. van Haarlem
Netherlands Institute for Radio Astronomy (ASTRON)
M. Hoeft
Thüringer Landessternwarte Tautenburg
A. J. van der Horst
George Washington University
E. Jutte
Ruhr-Universität Bochum
M. Kadler
Julius-Maximilians Universität Würzburg
L.V.E. Koopmans
Rijksuniversiteit Groningen
A. Krankowski
University of Warmia and Mazury in Olsztyn
G. Mann
Leibniz-Institut Für Astrophysik Potsdam
A. Nelles
Deutsches Elektronen-Synchrotron (DESY)
Friedrich-Alexander-Universität Erlangen Nurnberg (FAU)
J. B. R. Oonk
Surfsara Bv
E. Orrú
Netherlands Institute for Radio Astronomy (ASTRON)
H. Paas
Rijksuniversiteit Groningen
V. N. Pandey
Netherlands Institute for Radio Astronomy (ASTRON)
R. Pizzo
Netherlands Institute for Radio Astronomy (ASTRON)
M. Pandey-Pommier
Université de Lyon
W. Reich
Max-Planck-Gesellschaft
Hanna Rothkaehl
Polish Academy of Sciences
Mark Ruiter
Netherlands Institute for Radio Astronomy (ASTRON)
D. J. Schwarz
Universität Bielefeld
A. Shulevski
Universiteit Van Amsterdam
Universiteit Leiden
M. Soida
Uniwersytet Jagiellonski w Krakowie
M. Tagger
Universite d'Orleans
C. Vocks
Leibniz-Institut Für Astrophysik Potsdam
Ramj Wijers
Universiteit Van Amsterdam
S. J. Wijnholds
Netherlands Institute for Radio Astronomy (ASTRON)
O. Wucknitz
Max-Planck-Gesellschaft
P.M. Zarka
LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique
Station de Radioastronomie de Nançay
P. Zucca
Netherlands Institute for Radio Astronomy (ASTRON)
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 658 A1Ämneskategorier
Annan fysik
Signalbehandling
Datorseende och robotik (autonoma system)
DOI
10.1051/0004-6361/202140649