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Browsing by Author "Kramer, M"

Browsing by Author "Kramer, M"

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  • Double pulsar system J0737-039 and its low-frequency observations with GMRT 
    Joshi, B. C; McLaughlin, M. A; Lyne, A. G; Kramer, M; Lorimer, D. R; Manchester, R. N; Camilo, F; Burgay, M; Possenti, A; Amico, N. D; Freire, P. C. C (Astronomical Society of India, 2004-09)
    The recent discovery of two radio pulsars, with periods of 23 ms and 2.8 s, in a tight 2.4 hour highly relativistic double neutron star binary, is one of the most significant discoveries of pulsar astronomy (Burgay et al. ...
  • A high Galactic latitude search for pulsars 
    Joshi, B. C; Burgay, M; Lyne, A. G; Manchester, R. N; Possenti, A; Camilo, F; Amico, N. D; Kramer, M (Astronomical Society of India, 2002-09)
    Millisecond pulsars (MSPs) are an important class of radio pulsars. Their observed spatial distribution is flux limited and is nearly isotropic. Many such pulsars have been observed at high Galactic latitudes. The ...
  • Next Generation Software Based Instruments for Pulsar Astronomy 
    Joshi, B. C; Lyne, A. G; Kramer, M (Astronomical Society of India, 2003)
    High time resolution studies of pulsars require specialized instrumentation to counter the degradation in the quality and time resolution of their radio signals due to dispersion in the inter-stellar medium. The availability ...
  • On the usefulness of existing solar wind models for pulsar timing corrections 
    Tiburzi, C; Verbiest, J. P. W; Shaifullah, G. M; Janssen, G. H; Anderson, J. M; Horneffer, A; Kunsemoller, J; Ostowski, S; Donner, J. Y; Kramer, M; Anshu Kumari; Porayko, N. K; Zucca, P; Ciardi, B; Dettmar, R.J; Griebmeier, J.M; Hoeft, M; Serylak, M (Oxford University Press on behalf of the Royal Astronomical Society, 2019-07)
    Dispersive delays due to the solar wind introduce excess noise in high-precision pulsar timing experiments, and must be removed in order to achieve the accuracy needed to detect, e.g., low-frequency gravitational waves. ...
  • Role of time resolution on polarization of pulsar radiation 
    Gangadhara, R. T; Xilouris, K. M; von Hoensbroech, A; Kramer, M; Jessner, A; Wielebinski, R (The European Southern Observatory, 1999-02)
    The role of orthogonal polarization modes in pulsar emission is re-examined in view of polarization data of high time resolution. Individual pulse data of PSR B1133+16 at 1.41 GHz, obtained with time resolutions of 1160, ...

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