Polarized point sources in the LOFAR Two-meter Sky Survey: A preliminary catalog
Reviewartikel, 2018
The polarization properties of radio sources at very low frequencies (<200 MHz) have not been widely measured, but the new generation of low-frequency radio telescopes, including the Low Frequency Array (LOFAR: a Square Kilometre Array Low pathfinder), now gives us the opportunity to investigate these properties. In this paper, we report on the preliminary development of a data reduction pipeline to carry out polarization processing and Faraday tomography for data from the LOFAR Two-meter Sky Survey (LOTSS) and present the results of this pipeline from the LOTSS preliminary data release region (10h45m–15h30m right ascension, 45°–57° declination, 570 square degrees). We have produced a catalog of 92 polarized radio sources at 150 MHz at 4.′3 resolution and 1 mJy rms sensitivity, which is the largest catalog of polarized sources at such low frequencies. We estimate a lower limit to the polarized source surface density at 150 MHz, with our resolution and sensitivity, of 1 source per 6.2 square degrees. We find that our Faraday depth measurements are in agreement with previous measurements and have significantly smaller errors. Most of our sources show significant depolarization compared to 1.4 GHz, but there is a small population of sources with low depolarization indicating that their polarized emission is highly localized in Faraday depth. We predict that an extension of this work to the full LOTSS data would detect at least 3400 polarized sources using the same methods, and probably considerably more with improved data processing.
ISM: magnetic fields
Polarization
Författare
C.L. Van Eck
Radboud Universiteit
M. Haverkorn
Radboud Universiteit
M.I.R. Alves
Radboud Universiteit
R. Beck
Max-Planck-Gesellschaft
P.N. Best
University of Edinburgh
E. Carretti
Istituto nazionale di astrofisica (INAF)
K. Chyzy
Uniwersytet Jagiellonski w Krakowie
J.S. Farnes
Radboud Universiteit
K. Ferriere
Université de Toulouse
M. J. Hardcastle
University of Hertfordshire
G. Heald
Rijksuniversiteit Groningen
Commonwealth Scientific and Industrial Research Organisation (CSIRO)
Cathy Horellou
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
M. Iacobelli
Netherlands Institute for Radio Astronomy (ASTRON)
V. Jelic
Ruđer Bošković Institutet
D.D. Mulcahy
University of Manchester
S. O'Sullivan
Universität Hamburg
I.M. Polderman
Radboud Universiteit
Wolfgang Reich
Max-Planck-Gesellschaft
C. J. Riseley
Commonwealth Scientific and Industrial Research Organisation (CSIRO)
H.J.A. Rottgering
Universiteit Leiden
D.H.F.M. Schnitzeler
Max-Planck-Gesellschaft
T. W. Shimwell
Netherlands Institute for Radio Astronomy (ASTRON)
Universiteit Leiden
V. Vacca
Istituto nazionale di astrofisica (INAF)
J. Vink
Universiteit Van Amsterdam
G. J. White
RAL Space/STFC
Open University
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 613 A58Ämneskategorier
Subatomär fysik
Astronomi, astrofysik och kosmologi
Annan fysik
Fundament
Grundläggande vetenskaper
DOI
10.1051/0004-6361/201732228