Simultaneous single-pulse observations of radio pulsars: I. The polarization characteristics of PSR B0329+54
arXiv:astro-ph/0109507 · doi:10.1051/0004-6361:20011306
Abstract
We present the first results from a programme of multi-frequency simultaneous single pulse observations carried out as part of the European Pulsar Network. We detail the main data analysis methods and apply them to simultaneous observations of the strong pulsar B0329+54 at 1.4 and 2.7 GHz using the Jodrell Bank and Effelsberg radio telescopes respectively. The pulses at different frequencies are highly correlated in their total intensity, as seen in previous experiments, and generally show consistent position angles of the linearly polarized component. In contrast, the circularly polarized emission sometimes shows clear differences between pulses received at different frequencies. These results are unexpected and warrant further follow-up studies to interpret them in the context of the intrinsic bandwidth of pulsar radiation.
arXiv commentTo be published in A&A. 8 pages, 7 figures
References in corpus (5)
- The characteristics of millisecond pulsar emission: III.From low to high frequencies
- Polarization Sweeps in Rotation Powered Pulsars
- Circular polarization in pulsar integrated profiles
- Simultaneous Dual Frequency Observations of Giant Pulses from the Crab Pulsar
- A flexible format for exchanging pulsar data
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