Free access
Issue
Astron. Astrophys. Suppl. Ser.
Volume 127, Number 3, February I 1998
Page(s) 355 - 366
DOI http://dx.doi.org/10.1051/aas:1998106
DOI: 10.1051/aas:1998106

A&A Supplement series, Vol. 127, February I 1998, 355-366

Received February 3; accepted May 23, 1997

Catalogue of time aligned profiles of 56 pulsars at frequencies between 102 and 10500 MHz

A.D. Kuzmintex2html_wrap493 - V.A. Izvekovatex2html_wrap493 - Yu.P. Shitovtex2html_wrap493 - W. Siebertex2html_wrap499 - A. Jessnertex2html_wrap501 - R. Wielebinskitex2html_wrap501 - A.G. Lynetex2html_wrap505 - F.G. Smithtex2html_wrap505

Send offprint request: W. Sieber

tex2html_wrap509  Dept. of Radio Astronomy, Astro Space Center of Lebedev Physical Institute, Leninski Prospect 53, Moscow 117924, Russia
tex2html_wrap511  Fachhochschule Niederrhein, Reinarzstrasse 49, D-47805, Krefeld, Germany
tex2html_wrap513  Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
tex2html_wrap515  University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, UK

Abstract:

A catalogue of integrated pulse profiles of 56 pulsars with observations at 102, 230, 408, 610, 1400, 4700, and 10500 MHz is presented. The profiles are aligned in time (phase) so that direct comparisons of changes in the profile shape and component composition can be made. Smearing due to interstellar scattering at low frequencies for pulsars with large dispersion measures was removed by means of a special "descattering" method (Kuzmin & Izvekova 1993).

Most pulsars show good alignment over the whole frequency range 0.1 to 10.5 GHz, if the dispersion measure is corrected slightly in comparison to the published value. We confirm a non-dispersive time shift of the integrated profile for PSR 0809+74 as presented by Bartel et al. (1981), Davies et al. (1984), and Kuzmin et al. (1986).

This paper presents the data in form of a catalogue of time aligned profiles. A detailed analysis of the change of pulse structure with frequency by means of a decomposition of the average pulse shape into gaussian components will be presented in a forthcoming paper.

keywords: pulsars: general

SIMBAD Objects

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