J
John Reynolds
Researcher at Australia Telescope National Facility
Publications - 166
Citations - 6624
John Reynolds is an academic researcher from Australia Telescope National Facility. The author has contributed to research in topics: Very-long-baseline interferometry & Pulsar. The author has an hindex of 42, co-authored 166 publications receiving 6355 citations. Previous affiliations of John Reynolds include Max Planck Society & ASTRON.
Papers
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Journal ArticleDOI
The VSOP 5 GHz AGN Survey I. Compilation and Observations
Hisashi Hirabayashi,Edward B. Fomalont,Shinji Horiuchi,James E. J. Lovell,G. A. Moellenbrock,Makoto Inoue,Bernard F. Burke,Peter E. Dewdney,Leonid I. Gurvits,Hideyuki Kobayashi,David L. Jauncey,Yasuhiro Murata,P. M. McCulloch,Robert A. Preston,I. M. Avruch,Philip G. Edwards,Sean M. Dougherty,W. K. Scott,Sándor Frey,Zsolt Paragi,Yuri Kovalev,M. V. Popov,Jonathan D. Romney,Richard Schilizzi,Zhi-Qiang Shen,George D. Nicolson,Jonathan Quick,M. E. Costa,Richard Dodson,John Reynolds,Anastasios Tzioumis,Steven Tingay,X. Y. Hong,Shi Guang Liang,Xin Yong Huang,Wen Ren Wei,Corrado Trigilio,Gino Tuccari,Junichi Nakajima,Eiji Kawai,Tomofumi Umemoto,Takeshi Miyaji,Kenta Fujisawa,Noriyuki Kawaguchi,Andrzej Kus,Frank D. Ghigo,Chris Salter,Tapasi Ghosh,B. Z. Kanevsky,V. I. Slysh,A. G. Gunn,Paul Burgess,B. Carlson,David Del Rizzo,Russ Taylor,Wayne Cannon,Seiji Kameno,Kazunori M. Shibata,J. M. Benson,Chris Flatters,Andrew Hale,Craig Lewis,Glen Langston,Anthony H. Minter,Kevin Miller,Joel Smith,Richard Wietfeldt,Valery Altunin,David L. Meier,David W. Murphy,George Resch,Matthew L. Lister,B. Glenn Piner,Robert Jenkins,James Border,Jesus Gimeno +75 more
TL;DR: The VSOP Survey as mentioned in this paper was a Japanese-led project to image radio sources with sub-milliarcsec resolution by correlating the signal from the orbiting 8-m telescope, HALCA, with a global array of telescopes.
Journal ArticleDOI
Observations and modeling of relativistic spin precession in psr j1141–6545
R. N. Manchester,Michael Kramer,Michael Kramer,Ingrid H. Stairs,Ingrid H. Stairs,Ingrid H. Stairs,M. Burgay,Fernando Camilo,George Hobbs,Duncan R. Lorimer,Andrew Lyne,Maura McLaughlin,Christie A. McPhee,A. Possenti,John Reynolds,W. van Straten +15 more
TL;DR: The Parkes radio telescope has been used to observe the binary pulsar PSR J1141-6545 for 9.3 years as discussed by the authors, and the results show that the P.A. variations, both across the pulse profile and over the data span, are complex, with major differences between the central and outer parts of the pulse profiles.
Journal ArticleDOI
VSOP Space VLBI and Geodetic VLBI Investigations of Southern Hemisphere Radio Sources
Steven Tingay,Steven Tingay,John Reynolds,Anastasios Tzioumis,David L. Jauncey,James E. J. Lovell,Richard Dodson,M. E. Costa,P. M. McCulloch,P. G. Edwards,Hisashi Hirabayashi,David W. Murphy,Robert A. Preston,B. G. Piner,George D. Nicolson,J. F. H. Quick,Hideyuki Kobayashi,Katsunori Shibata +17 more
TL;DR: In this article, images from VLBI Space Observatory Programme (VSOP) observations of 14 compact extragalactic southern hemisphere radio sources were presented, including a description of the observations, the data reduction techniques, and the parameters of the resulting images and model fits.
Journal ArticleDOI
The Nearest GHz Peaked-Spectrum Radio Galaxy, PKS 1718-649
Steven Tingay,D. L. Jauncey,John Reynolds,Anastasios Tzioumis,E. A. King,Robert A. Preston,James E. J. Lovell,P. M. McCulloch,M. E. Costa,George D. Nicolson,Anton M. Koekemoer,Merja Tornikoski,Lucyna Kedziora-Chudczer,D. Campbell-Wilson +13 more
TL;DR: In this paper, the authors identify PKS 1718-649, at a distance of 56 Mpc (z = 0.014; H(sub o) = 75 km/s/Mpc, q(sub O) = 0), as the nearest GHz peaked-spectrum (GPS) radio galaxy, more than four times closer than any previously known.
Journal ArticleDOI
Structure of the radio remnant of supernova 1987A
Lister Staveley-Smith,D. S. Briggs,Alistair Rowe,R. N. Manchester,John Reynolds,Anastasios Tzioumis,Michael Kesteven +6 more
TL;DR: In this article, high-resolution images of the supernova remnant at a frequency of 8.8 GHz were presented, which reveal a spherical shell-like structure with a radius of 0.6 arcsec (4 × 1017 cm, assuming a distance of 50 kpc) and an additional component that is aligned with the optical ring.