Pulse profiles and timing of PSR J1757$-$2421

Abstract

Pulse arrival time measurements over fourteen years with the Nanshan 25-m and Parkes 64-m radio telescopes have been used to determine the average profile and timing properties for PSR J1757$-$2421 (B1754$-$24). Analysis of the radio profile data shows a large variation of spectral index across the profile and an unusual increase in component separation with increasing frequency. The timing observations show that PSR B1754$-$24 underwent a large glitch with a fractional increase in spin frequency of $\Delta {\nu }_{\mathrm{g}}/\nu \sim 7.8\times 10^{-6}$ in May 2011. At the time of the glitch there was a large permanent jump in the rotational frequency accompanied by two exponential recovery terms with timescales of 15(6) and 97(15) days, respectively.

9 pages, 8 figures, 5 tables, Accepted for publication in MNRAS

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• A short review of the pulsar magnetic inclination angles (II)
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• Measuring the crust-superfluid coupling time-scale for 105 UTMOST pulsars with a Kalman filter