E. Koerding
Max Planck Society
4 Papers
E. Koerding is an academic researcher from Max Planck Society. The author has contributed to research in topics: Jet (fluid) & Magnitude (astronomy). The author has an hindex of 1, co-authored 1 publications.
Chat about Author
Papers
Radio jet precession in M81*
S. von Fellenberg,Michael Janssen,Jordy Davelaar,Michal Zajacek,Silke Britzen,Heino Falcke,E. Koerding,Elisa Da Ros +7 more
TL;DR: In this paper , position angle measurements of the core region of M81* at 5 GHz and 8 GHz were reported, which confirm the presence of sinusoidal jet precession of the M81 jet region as suggested by Marti-Vidal2011.
16
Swift J1727.8-1613 has the Largest Resolved Continuous Jet Ever Seen in an X-ray Binary
Callan M. Wood,J. Miller-Jones,Arash Bahramian,S. Tingay,Steve Prabu,T. D. Russell,P. Atri,F. Carotenuto,D. Altamirano,S. Motta,L. Hyland,Cormac Reynolds,Stuart Weston,Robert Fender,E. Koerding,Dipankar Maitra,Sera Markoff,Simone Migliari,D. Russell,Craig L. Sarazin,Gregory R. Sivakoff,R. Soria,Alexandra J. Tetarenko,Valeriu Tudose +23 more
- 20 May 2024
TL;DR: Researchers observe Swift J1727.8-1613, an X-ray binary, using the Very Long Baseline Array and Long Baseline Array, revealing a large, two-sided, resolved jet extending 110 AU, with a lower limit on the jet speed of 0.27c and upper limit on jet inclination of 74 degrees.
4
Identifying and characterising the population of hot sub-luminous stars with multi-colour MeerLICHT data
P. Ranaivomanana,Cole Johnston,Paul J. Groot,Conny Aerts,Rebecca Nicole Lees,L. IJspeert,Steven Bloemen,M. Klein-Wolt,Patrick A. Woudt,E. Koerding,R. S. Le Poole,D. L. A. Pieterse +11 more
- 14 Feb 2023
TL;DR: In this paper , MeerLICHT was used to detect hot sub-luminous stars and identify the dominant frequency in the photometric variability of these compact hot stars in comparison to their $Gaia$ DR3 data.
Very Long Baseline Interferometry with the SKA
Zsolt Paragi,Leith Godfrey,C. Reynolds,Maria Rioja,Adam Deller,B. Zhang,L. Gurvits,M. Bietenholz,A. Szomoru,H. E. Bignall,P. Boven,P. Charlot,Richard Dodson,Sándor Frey,M. A. Garrett,Hiroshi Imai,A. P. Lobanov,M. J. Reid,Eduardo Ros,H. J. van Langevelde,Anton Zensus,X. W. Zheng,A. Alberdi,Iván Agudo,Tao An,Megan Argo,Robert Beswick,A. Biggs,Andreas Brunthaler,B. Campbell,Giuseppe Cimo,F. Colomer,S. Corbel,John Conway,D. Cseh,Roger Deane,Heino Falcke,Marcin P. Gawronski,M. Gaylard,Gabriele Giovannini,Marcello Giroletti,Ciriaco Goddi,Sharmila Goedhart,José L. Gómez,A. Gunn,Preeti Kharb,H. R. Kloeckner,E. Koerding,Yuri Y. Kovalev,Magdalena Kunert-Bajraszewska,Michael Lindqvist,Matthew L. Lister,F. Mantovani,Ivan Marti-Vidal,M. Mezcua,John McKean,Enno Middelberg,James Miller-Jones,J. Moldon,T. W. B. Muxlow,Tim O'Brien,Miguel A. Pérez-Torres,S. V. Pogrebenko,J. Quick,A. Rushton,R. Schilizzi,O. Smirnov,Bong Won Sohn,G. Surcis,G. B. Taylor,Steven Tingay,V. M. Tudose,A. J. van der Horst,J. van Leeuwen,Tiziana Venturi,R. Vermeulen,Wouter Vlemmings,A. de Witt,Olaf Wucknitz,Jun Yang,Krisztina É. Gabányi,T. Jung +81 more
- 29 May 2015
TL;DR: In this article, the authors proposed a VLBI capability to the SKA arrays, which can greatly broaden the science of SKA, and is feasible within the current specifications, and can be implemented by providing phased-array outputs for SKA1-MID and SKA 1-SUR and using these extremely sensitive stations with other radio telescopes.