Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-12T14:38:46.859Z Has data issue: false hasContentIssue false

Pulsar Timing at the Radiotelescope Effelsberg

Published online by Cambridge University Press:  12 April 2016

Ch. Lange
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, Germany
N. Wex
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, Germany
M. Kramer
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, Germany
O. Doroshenko
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, Germany
D.C. Backer
Affiliation:
Astronomy Department, University of California, Berkeley, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present results of timing observations, obtained at the 100 m-Radiotelescope Effelsberg since 1994. The quality of the pulse arrival times, recorded with the coherent de-disperser EBPP since October 1996, is excellent. Our TOAs are well suited for the measurement of binary parameters of binary pulsars with short orbital periods. Some results are presented.

Type
Part 2. Timing, General Relativity and Astrometry
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Backer, D.C., Dexter, M.R., Zepka, A., Ng, D., Werthimer, D.J., Ray, P.S., Foster, R.S., 1997, Publ. Astr. Soc. Pacific, 109, 61 Google Scholar
Rawley, L.A., 1986, PhD-thesis, Princeton University Google Scholar
Taylor, J.H., 1992, Phil. Trans. Roy. Soc. London A, 341, 117 Google Scholar
Toscano, M., Sandhu, J.S., Bailes, M., Manchester, R.N., Britton, M.C., Kulkarni, S.R., Anderson, S.B., Stappers, B.W., 1999, MNRAS, 307, 925 CrossRefGoogle Scholar
Wex, N., 2000, these proceedingsGoogle Scholar