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First e-VLBI observations of GRS 1915+105

Published online by Cambridge University Press:  01 August 2006

A. Rushton
Affiliation:
The University of Manchester, Jodrell Bank Observatory, Cheshire SK11 9DA, UK email: [email protected]
R. E. Spencer
Affiliation:
The University of Manchester, Jodrell Bank Observatory, Cheshire SK11 9DA, UK email: [email protected]
M. Strong
Affiliation:
The University of Manchester, Jodrell Bank Observatory, Cheshire SK11 9DA, UK email: [email protected]
R. M. Campbell
Affiliation:
Joint Institute for VLBI in Europe, Postbus 2, 7990 A A Dwingeloo, The Netherlands
S. Casey
Affiliation:
The University of Manchester, Jodrell Bank Observatory, Cheshire SK11 9DA, UK email: [email protected]
R. P. Fender
Affiliation:
School of Physics and Astronomy, University of Southampton, Southampton, UK “Anton Pannekoek” Astronomical Inst., Univ. of Amsterdam, Amsterdam, The Netherlands
M. A. Garrett
Affiliation:
Joint Institute for VLBI in Europe, Postbus 2, 7990 A A Dwingeloo, The Netherlands
J. C. A. Miller-Jones
Affiliation:
“Anton Pannekoek” Astronomical Inst., Univ. of Amsterdam, Amsterdam, The Netherlands
G. G. Pooley
Affiliation:
University of Cambridge, Mullard Radio Astronomy Observatory, CB3 0HE Cambridge, UK
C. Reynolds
Affiliation:
Joint Institute for VLBI in Europe, Postbus 2, 7990 A A Dwingeloo, The Netherlands
A. Szomoru
Affiliation:
Joint Institute for VLBI in Europe, Postbus 2, 7990 A A Dwingeloo, The Netherlands
V. Tudose
Affiliation:
“Anton Pannekoek” Astronomical Inst., Univ. of Amsterdam, Amsterdam, The Netherlands Astronomical Institute of the Romanian Academy, Cutitul de Argint 5, Bucharest, Romania
Z. Paragi
Affiliation:
Joint Institute for VLBI in Europe, Postbus 2, 7990 A A Dwingeloo, The Netherlands
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Abstract

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We present results from the first successful open call e-VLBI science run, observing the X-ray binary GRS 1915+105. e-VLBI science allows the rapid production of VLBI radio maps, within hours of an observation rather than weeks. A total of 6 telescopes observing at 5 GHz across the European VLBI Network (EVN) were correlated in real time at the Joint Institute for VLBI in Europe (JIVE). Throughout this, GRS 1915+105 was observed for a total of 5.5 hours, producing 2.8 GB of visibilities of correlated data. The peak brightness was 10.2 mJy per beam, with a total integrated radio flux of 11.1 mJy.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

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