Calibrating high-precision Faraday rotation measurements for LOFAR and the next generation of low-frequency radio telescopes (Corrigendum)

C. Sotomayor-Beltran; C. Sobey; J. W. T. Hessels; G. de Bruyn; A. Noutsos; A. Alexov; J. Anderson; A. Asgekar; I. M. Avruch; R. Beck; M. E. Bell; M. R. Bell; M. J. Bentum; G. Bernardi; P. Best; L. Birzan; A. Bonafede; F. Breitling; J. Broderick; W. N. Brouw; M. Brüggen; B. Ciardi; F. de Gasperin; R.-J. Dettmar; A. van Duin; S. Duscha; J. Eislöffel; H. Falcke; R. A. Fallows; R. Fender; C. Ferrari; W. Frieswijk; M. A. Garrett; J. Grießmeier; T. Grit; A. W. Gunst; T. E. Hassall; G. Heald; M. Hoeft; A. Horneffer; M. Iacobelli; E. Juette; A. Karastergiou; E. Keane; J. Kohler; M. Kramer; V. I. Kondratiev; L. V. E. Koopmans; M. Kuniyoshi; G. Kuper; J. van Leeuwen; P. Maat; G. Macario; S. Markoff; J. P. McKean; D. D. Mulcahy; H. Munk; E. Orru; H. Paas; M. Pandey-Pommier; M. Pilia; R. Pizzo; A. G. Polatidis; W. Reich; H. Röttgering; M. Serylak; J. Sluman; B. W. Stappers; M. Tagger; Y. Tang; C. Tasse; S. ter Veen; R. Vermeulen; R. J. van Weeren; R. A. M. J.  Wijers; S. J. Wijnholds; M. W. Wise; O. Wucknitz; S. Yatawatta; P. Zarka

doi:10.1051/0004-6361/201220728e

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Erratum

This article is an erratum for: [this article]

Issue		A&A Volume 581, September 2015


Article Number		C4
Number of page(s)		2
Section		Astronomical instrumentation
DOI		https://doi.org/10.1051/0004-6361/201220728e
Published online		17 September 2015

A&A 581, C4 (2015)

Calibrating high-precision Faraday rotation measurements for LOFAR and the next generation of low-frequency radio telescopes (Corrigendum)

C. Sotomayor-Beltran¹, C. Sobey², J. W. T. Hessels³^,4, G. de Bruyn³^,5, A. Noutsos², A. Alexov⁴^,6, J. Anderson², A. Asgekar³, I. M. Avruch⁷^,5^,3, R. Beck², M. E. Bell⁸^,9, M. R. Bell¹⁰, M. J. Bentum³, G. Bernardi⁵, P. Best¹¹, L. Birzan¹², A. Bonafede¹³^,14, F. Breitling¹⁵, J. Broderick⁹, W. N. Brouw³^,5, M. Brüggen¹³, B. Ciardi¹⁰, F. de Gasperin¹³^,10, R.-J. Dettmar¹, A. van Duin³, S. Duscha³, J. Eislöffel¹⁶, H. Falcke¹⁷^,3, R. A. Fallows³, R. Fender⁹, C. Ferrari¹⁸, W. Frieswijk³, M. A. Garrett³^,12, J. Grießmeier³^,19, T. Grit³, A. W. Gunst³, T. E. Hassall⁹^,20, G. Heald³, M. Hoeft¹⁶, A. Horneffer², M. Iacobelli¹², E. Juette¹, A. Karastergiou²¹, E. Keane², J. Kohler², M. Kramer²^,20, V. I. Kondratiev³^,22, L. V. E. Koopmans⁵, M. Kuniyoshi², G. Kuper³, J. van Leeuwen³^,4, P. Maat³, G. Macario¹⁸, S. Markoff⁴, J. P. McKean³, D. D. Mulcahy², H. Munk³, E. Orru³^,17, H. Paas²³, M. Pandey-Pommier¹²^,24, M. Pilia³, R. Pizzo³, A. G. Polatidis³, W. Reich², H. Röttgering¹², M. Serylak¹⁹^,25, J. Sluman³, B. W. Stappers²⁰, M. Tagger¹⁹, Y. Tang³, C. Tasse²⁶, S. ter Veen¹⁷, R. Vermeulen³, R. J. van Weeren²⁷^,12^,3, R. A. M. J. Wijers⁴, S. J. Wijnholds³, M. W. Wise³^,4, O. Wucknitz²⁸^,2, S. Yatawatta³ and P. Zarka²⁶

¹ Astronomisches Institut der Ruhr-Universität Bochum, Universitätsstr. 150, 44780 Bochum, Germany
e-mail: sotomayor@astro.rub.de
² Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
³ ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA Dwingeloo, The Netherlands
⁴ Astronomical Institute “Anton Pannekoek,” University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands
⁵ Kapteyn Astronomical Institute, PO Box 800, 9700 AV Groningen, The Netherlands
⁶ Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
⁷ SRON Netherlands Insitute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
⁸ ARC Centre of Excellence for All-sky astrophysics (CAASTRO), Sydney Institute of Astronomy, University of Sydney Australia, Redfern NSW 2016, Australia
⁹ School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UK
¹⁰ Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, 85741 Garching, Germany
¹¹ Institute for Astronomy, University of Edinburgh, Royal Observatory of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK
¹² Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands
¹³ University of Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany
¹⁴ Jacobs University Bremen, Campus Ring 1, 28759 Bremen, Germany
¹⁵ Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
¹⁶ Thüringer Landessternwarte, Sternwarte 5, 07778 Tautenburg, Germany
¹⁷ Department of Astrophysics/IMAPP, Radboud University Nijmegen, PO Box 9010, 6500 GL Nijmegen, The Netherlands
¹⁸ Laboratoire Lagrange, UMR 7293, Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, 06300 Nice, France
¹⁹ Laboratoire de Physique et Chimie de l’Environnement et de l’Espace, LPC2E UMR 7328 CNRS, 45071 Orléans Cedex 02, France
²⁰ Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
²¹ Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH
²² Astro Space Center of the Lebedev Physical Institute, Profsoyuznaya str. 84/32, 117997 Moscow, Russia
²³ Center for Information Technology (CIT), University of Groningen, 9712 CP Groningen, The Netherlands
²⁴ Centre de Recherche Astrophysique de Lyon, Observatoire de Lyon, 9 Av. Charles André, 69561 Saint-Genis Laval Cedex, France
²⁵ Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU, 18330 Nançay, France
²⁶ LESIA, UMR CNRS 8109, Observatoire de Paris, 92195 Meudon, France
²⁷ Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
²⁸ Argelander-Institut für Astronomie, University of Bonn, Auf dem Hügel 71, 53121 Bonn, Germany

Key words: polarization / techniques: polarimetric / errata, addenda

Erratum to: A&A 552, A58 (2013), DOI: 10.1051/0004-6361/201220728

Fig. 2

GIMs representing the VTEC across the globe for April 11th, 2011 (the date of the first LOFAR observing campaign, see Sect. 5) obtained courtesy of CODE. The maps range from minimum (blue) to maximum (red) VTEC values of 0.0−87.2 TECU (1 TECU = 10¹⁶ electrons/m²). The triangles indicate the location of the LOFAR core stations in the Netherlands, the squares mark the SKA core sites in South Africa and Western Australia, and the circles indicate the site of the GMRT.

Open with DEXTER

This erratum corrects Figs. 2 and 3 of our original paper (Sotomayor-Beltran et al. 2013). Due to a simple error in plotting the input data, these maps of ionospheric total electron content (TEC) were inverted north-south and improperly stretched to match the underlying cartographic projection. The properly mapped figures are presented here (see also the Appendix of Arora et al. 2015). The ionospheric prediction code, ionFR, and other figures presented in the paper were not affected by this

	Fig. 3 The VTEC across Europe for March 23rd, 2012 (the date of the third LOFAR campaign, see Sect. 5) at 00:00 UT, obtained courtesy of ROB. The square indicates the LOFAR core stations and the triangles represent the locations of the international stations.
Open with DEXTER

inversion error, which was purely a plotting error applying to Figs. 2 and 3.

This mapping error led to the incorrect conclusion that the Equatorial Ionization Anomaly (EIA) can sometimes pass directly over the planned sites of the Square Kilometre Array (SKA). Though ionospheric calibration is a challenging problem, it is a challenge that is being met (e.g., Arora et al. 2015). Unfortunately, the incorrect assertion that the EIA passes over the chosen sites for the SKA overstated the severity of the problem for these locations, which have been meticulously chosen and proven to be excellent sites for low-frequency radio astronomy.

All other conclusions in the paper remain unaffected.

Acknowledgments

We sincerely thank David Herne, Mervyn Lynch, and John Kennewell for discovering this error and bringing it to our attention.

References

Arora, B. S., Morgan, J., Ord, S. M., et al. 2015, PASA, 32, 029 [NASA ADS] [CrossRef] [Google Scholar]
Sotomayor-Beltran, C., Sobey, C., Hessels, J. W. T., et al. 2013, A&A, 552, A58 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

© ESO, 2015

All Figures

	Fig. 2 GIMs representing the VTEC across the globe for April 11th, 2011 (the date of the first LOFAR observing campaign, see Sect. 5) obtained courtesy of CODE. The maps range from minimum (blue) to maximum (red) VTEC values of 0.0−87.2 TECU (1 TECU = 10¹⁶ electrons/m²). The triangles indicate the location of the LOFAR core stations in the Netherlands, the squares mark the SKA core sites in South Africa and Western Australia, and the circles indicate the site of the GMRT.
Open with DEXTER
In the text

	Fig. 3 The VTEC across Europe for March 23rd, 2012 (the date of the third LOFAR campaign, see Sect. 5) at 00:00 UT, obtained courtesy of ROB. The square indicates the LOFAR core stations and the triangles represent the locations of the international stations.
Open with DEXTER
In the text

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[1] Arora, B. S., Morgan, J., Ord, S. M., et al. 2015, PASA, 32, 029 [NASA ADS] [CrossRef] [Google Scholar]

[2] Sotomayor-Beltran, C., Sobey, C., Hessels, J. W. T., et al. 2013, A&A, 552, A58 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]