A transient component in the pulse profile of PSR J0738-4042

TL;DR

This paper reports the discovery of a transient component in the pulse profile of PSR J0738-4042, challenging the assumption of constant pulse profiles in pulsar timing and introducing a statistical method for detecting such changes.

Contribution

It presents the first detection of a transient pulse component in PSR J0738-4042 and introduces a Hidden Markov Model-based technique for identifying profile variations.

Findings

Transient component appeared between 2004 and 2006

Component's polarization properties align with orthogonal polarization modes

Statistical technique successfully detects low S/N profile changes

Abstract

One of the tenets of the radio pulsar observational picture is that the integrated pulse profiles are constant with time. This assumption underpins much of the fantastic science made possible via pulsar timing. Over the past few years, however, this assumption has come under question with a number of pulsars showing pulse shape changes on a range of timescales. Here, we show the dramatic appearance of a bright component in the pulse profile of PSR J0738-4042 (B0736-40). The component arises on the leading edge of the profile. It was not present in 2004 but strongly present in 2006 and all observations thereafter. A subsequent search through the literature shows the additional component varies in flux density over timescales of decades. We show that the polarization properties of the transient component are consistent with the picture of competing orthogonal polarization modes. Faced with the general problem of identifying and characterising average profile changes, we outline and apply a statistical technique based on a Hidden Markov Model. The value of this technique is established through simulations, and is shown to work successfully in the case of low signal-to-noise profiles.