ORCID Profile
0000-0001-5273-9817
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Publisher: American Astronomical Society
Date: 11-2004
DOI: 10.1086/424819
Publisher: Oxford University Press (OUP)
Date: 18-10-2012
Publisher: American Astronomical Society
Date: 04-1998
DOI: 10.1086/300284
Publisher: American Astronomical Society
Date: 20-04-1998
DOI: 10.1086/305494
Publisher: American Astronomical Society
Date: 20-11-2004
DOI: 10.1086/424811
Publisher: Oxford University Press (OUP)
Date: 05-11-2012
Publisher: American Astronomical Society
Date: 27-09-2012
Publisher: American Astronomical Society
Date: 10-10-1996
DOI: 10.1086/310292
Publisher: American Astronomical Society
Date: 20-10-2000
DOI: 10.1086/317049
Publisher: American Astronomical Society
Date: 08-02-2012
Publisher: Springer Science and Business Media LLC
Date: 14-03-2013
Publisher: American Astronomical Society
Date: 14-12-2007
DOI: 10.1086/527300
Publisher: American Astronomical Society
Date: 11-1997
DOI: 10.1086/118621
Publisher: American Astronomical Society
Date: 04-2000
DOI: 10.1086/301283
Publisher: American Astronomical Society
Date: 10-07-2012
Publisher: Oxford University Press (OUP)
Date: 29-07-2014
Publisher: American Astronomical Society
Date: 10-09-2000
DOI: 10.1086/312875
Publisher: Oxford University Press (OUP)
Date: 07-2009
Publisher: EDP Sciences
Date: 06-2014
Publisher: American Astronomical Society
Date: 11-2004
DOI: 10.1086/424820
Publisher: Oxford University Press (OUP)
Date: 25-04-2006
Publisher: EDP Sciences
Date: 20-05-2011
Publisher: American Association for the Advancement of Science (AAAS)
Date: 18-09-1998
DOI: 10.1126/SCIENCE.281.5384.1825
Abstract: High angular resolution images of extragalactic radio sources are being made with the Highly Advanced Laboratory for Communications and Astronomy (HALCA) satellite and ground-based radio telescopes as part of the Very Long Baseline Interferometry (VLBI) Space Observatory Programme (VSOP). VSOP observations at 1.6 and 5 gigahertz of the milli–arc-second–scale structure of radio quasars enable the quasar core size and the corresponding brightness temperature to be determined, and they enable the motions of jet components that are close to the core to be studied. Here, VSOP images of the gamma-ray source 1156+295, the quasar 1548+056, the ultraluminous quasar 0014+813, and the superluminal quasar 0212+735 are presented and discussed.
Publisher: American Astronomical Society
Date: 03-2004
DOI: 10.1086/381957
Publisher: Oxford University Press (OUP)
Date: 21-07-2009
Publisher: EDP Sciences
Date: 30-01-2014
Publisher: Oxford University Press (OUP)
Date: 25-04-2003
Publisher: EDP Sciences
Date: 09-2010
Publisher: Oxford University Press (OUP)
Date: 1997
Publisher: EDP Sciences
Date: 09-2002
Publisher: Elsevier BV
Date: 2000
Publisher: Oxford University Press (OUP)
Date: 15-06-2010
Publisher: American Astronomical Society
Date: 04-12-2013
Publisher: American Astronomical Society
Date: 03-12-2013
Publisher: Springer Science and Business Media LLC
Date: 19-03-2014
Publisher: Oxford University Press (OUP)
Date: 13-07-2013
Publisher: American Astronomical Society
Date: 03-2005
DOI: 10.1086/427399
Publisher: EDP Sciences
Date: 09-2014
Publisher: EDP Sciences
Date: 30-03-2015
Publisher: Springer Science and Business Media LLC
Date: 12-2011
Publisher: American Astronomical Society
Date: 04-2008
DOI: 10.1086/525025
Publisher: American Astronomical Society
Date: 03-10-2006
DOI: 10.1086/507991
Publisher: American Astronomical Society
Date: 20-11-1998
DOI: 10.1086/311723
Publisher: EDP Sciences
Date: 09-2014
Publisher: Elsevier BV
Date: 2000
Publisher: American Astronomical Society
Date: 20-11-1996
DOI: 10.1086/310353
Publisher: Oxford University Press (OUP)
Date: 28-04-2013
DOI: 10.1093/MNRAS/STT558
Publisher: American Astronomical Society
Date: 08-2002
DOI: 10.1086/340783
Publisher: American Astronomical Society
Date: 15-10-2010
Publisher: Oxford University Press (OUP)
Date: 02-2009
Publisher: Oxford University Press (OUP)
Date: 10-2004
Publisher: American Astronomical Society
Date: 12-1997
DOI: 10.1086/304920
No related organisations have been discovered for James Lovell.
Start Date: 2015
End Date: 2015
Funder: Australian Research Council
View Funded ActivityStart Date: 2015
End Date: 2015
Funder: Geoscience Australia
View Funded ActivityStart Date: 2015
End Date: 2015
Funder: Max Planck Institute for Radio Astronomy
View Funded ActivityStart Date: 2015
End Date: 2015
Funder: Auckland University of Technology
View Funded ActivityStart Date: 2015
End Date: 2015
Funder: CSIRO-Commonwealth Scientific & Industrial Research Organisation
View Funded ActivityStart Date: 2015
End Date: 2015
Funder: Smithsonian Institution
View Funded ActivityStart Date: 2006
End Date: 2009
Funder: CSIRO-Commonwealth Scientific & Industrial Research Organisation
View Funded ActivityStart Date: 2010
End Date: 2013
Funder: Australian Research Council
View Funded ActivityStart Date: 2009
End Date: 2018
Funder: CSIRO-Commonwealth Scientific & Industrial Research Organisation
View Funded ActivityStart Date: 2007
End Date: 2013
Funder: Department of Industry and Science
View Funded Activity